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soxsick · 4 months
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reblog or just like.
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dailycass-cain · 2 months
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so this is my first time reading Batgirl (TYSM for the guide!) and I'm pretty new to comics in general. I've made it to #41 so far, and I can't help but notice the huge decline in writing from #38 onwards with the change of writers. Maybe it's just exacerbated by how good the previous issues were; but it really feels like Cass drastically went from a rare female character that is actually written with the same respect and depth as the male characters to being turned into a "girl superhero" with boy troubles who gets forced into bikinis and love triangles. Since you seem to know a lot about what was going on behind the scenes at the time, did something happen? I know there's misogynistic/racist men in the industry who hated Cass so I was wondering if that was already brewing back then during her 2000s run
I think when it came post-Puckett era, Dylan Horrocks was faced with a choice: ape off Puckett or try something different with the character.
I'll be honest, the early Horrocks' stuff you're in hasn't aged well. The ideas are interesting, of exploring sexuality and Cass realizing she can "see" what men think of her, and I think the utter realization of Babs making a mistake is good. It's just the overall execution is more of a miss.
The thing is, #41 gives us an excellent in-character reason for her choices. It's just this is all balanced with Bruce being pretty awful to Cass during this period (because this is all in a lead-up to Horrocks "big" story for #50).
Horrocks run can best be summed as: starts "meh" has interesting ideas, but fails to fully execute them well. There are some standoff amazing moments in the comics (I think the Doll Man issue is quite underrated).
Though, you're right. This is the era when Dan DiDio began to rise to power within the DC Comics Company, and it shows during this particular run.
So during this "run" we had A LOT of things happen outside the comic.
#1 Batman: Hush going on, and that story is particularly infamous for neglecting Cass due to story writer Jeph Loeb's distaste cause she wasn't Barbara Gordon (artist Jim Lee, who now currently runs DC too had this idea but since 2020 has softened this stance and realizes the mistake made).
Add this with DiDio's bias toward the Bronze Age "iconic" characters (Barry, Hal, and Babs) you have this growing problem.
#2 Cass DID get to be involved in another comic. The Justice League: Elite maxi-series. Though she didn't show up in THE Batman story, Cass was showing up in two other series at this time. One, well is in my "infamous" Cass reading guide (Batman: City of Light), and JL: Elite.
The later series did a nice job with the "twist" that Cass was on the team and as an agent of Batman spying on them. It is an actually interesting and good story.
#3 This is the era the "editorial edicts" started to come in. So a rather infamous thing during DiDio's reign was editorial edicts that would force changes in comics (leading to some outrageous OOC moments). This happened TWICE in Horrocks' Batgirl run.
At a certain point, Horrocks is told via top brass that he's losing Babs as a supporting cast member and has to write her off the comic. So he has to write a Babs/Cass go their separate ways due to well you'll see.
The other is in regards to Stephanie Brown who'll be back in the comic past #50 (she left the series in #38). What Horrocks didn't know until a Bat summit around this time (where all the Batman book creatives discussed where to take the books in the coming months) is that Stephanie's days were numbered.
She was coming back (and as Robin), but they were killing off the character. Horrocks and Nightwing writer Devin Grayson HATED the idea and objected to it.
Sadly, they were outvoted and well whatever else occurred in those meetings (or after) resulted in Horrocks quitting the Batgirl series and DC Comics itself by #57 (this is why Horrocks' run on the book just ends abruptly with no real end). Horrocks is still currently just enjoying the life of writing and doing Indie comics.
Interestingly, whatever Horrocks said or did it's interesting to note his is the only run never collected fully by DC Comics. Sadly, the only Batgirl issues that were EVER put in a trade were the stuff that made him walk (Batman: War Games, the event that killed Stephanie Brown). That was until the mid-2010s when DC released a HC Batgirl Anniversary trade that also included stories of Bette Kane, Steph, and Cass as Batgirl. #45 (aka Cass wearing Babs' Batgirl costume) is in the trade collection.
Ironically, this bad management editorial would also eventually affect Kelley Puckett (who returns to DC with Supergirl Vol. 5 #23-29, 31-32) around 2008 to 2009 but then ALSO decided to leave DC and comics altogether.
Not those two, but also the writer who'd replaced Horrocks, Andersen Gabrych (who was one of the minds behind War Games). However, I honestly do love Gabrych's run on Batgirl more than Horrocks. It's just the edicts and the rushing toward the end of his run kind of sours it.
I hope all this information is helpful.
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iconsfilm · 3 years
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like or reblog if you save
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katnissgirlsmakedo · 3 years
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question. do u have any remaining thoughts about DIARIES or is that a thing of the past
i love you so much <3 i DO have remaining thoughts! it could never be fully in the past although i have definitely calmed down a lot since june or whenever i was doing that (for those of you that weren’t here, DIARIES is a tv show i made up in my brain, think riverdale, that crosses diary of a wimpy kid and dork diaries and is about the two protagonists, greg and nikki, in college together, they meet they hate each other they become friends etc enemies to lovers slowburn four seasons and a movie)
i had an old (like 2 weeks not from all the way back in june) draft where i listed the endgame couples but i’ve since changed my stance on half of them and the only one that mattered anyway was nikki and greg <3 and also the great thing about the endgame is that literally everyone can hook up with each other along the way, god bless the broken road that led me straight to you etc etc. idk if i have any more general thoughts, i think i’ve said it all without being weirdly detailed, but i think you should all know that i have legitimately written a few little pieces of this tv show that doesn’t exist and probably won’t ever exist. so that’s where i’m at with it, having fun and making long tumblr posts and generally vibing until i can peer pressure everyone into watching or rewatching diary of a wimpy kid and the maybe possibly upcoming dork diaries movie that by my calculations has been “about to be made” for like five years at least. anyway.
oh yeah i also have the dream cast mostly visualized but i’m not going to make this post as annoying as adding pictures so just trust me on this list: yara shahidi as nikki, and i previously said griffin gluck as greg but tbh zachary gordon is only 23 and could totally reprise the role of his career. sofia wylie and jenna ortega as zoey and chloe, millie bobby brown as mackenzie (please trust that i have a vision on that one), matt cornett as brandon, i was about to think that saying marsai martin as brianna was too self indulgent but like this is literally my show in my brain. rowley is yet to be determined because my brain is big but not that big, devin bostick also reprises his iconic and career defining performance as rodrick, then mackenzie foy (of twilight demon baby fame) as patty- just trust the energy, and the guy from the after movies plays that weirdo fregley. for the laffs <3
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anhed-nia · 4 years
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BLOGTOBER 10/4/2020: SOCIETY
Without having a survey to back me up, I feel comfortable asserting that as a horror fan, you go through different phases with SOCIETY. It’s a basic fact of life, and yet it morphs and mutates underneath you, shocking you anew just when you think you’ve got a grip on it. You never forget your first time, because there is simply nothing like it. Then, after you get over the initial shock of its patented brand of body horror, you start to take it for granted; it's so broad and monolithic that it becomes something like the Grand Canyon--when it’s not right there in front of you, you begin to experience it more iconically, as part of the wallpaper of existence, rather than an in-your-face confrontation with the limits of experience. Then, you revisit it every few years (or months, depending on what sort of person you are), and the prophylactic layer that your brain has wrapped around your memories of it--the one that allows you to think of SOCIETY as a fun, wacky cheap thrill--begins to crumble, and you realize all over again how iconoclastically vile it is. Wherever you happen to be at, with this inimitable genre landmark, you'd be hard pressed to deny that it earns its royal status among horror movies, just for being so uniquely fucked up.
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Filmmaker Brian Yuzna is best known as the co-creator of the indispensable RE-ANIMATOR (or as the co-writer of HONEY, I SHRUNK THE KIDS...depending on what sort of person you are, again), itself a milestone achievement in the blending of sex and gore that so characterized '80s horror production. That film clearly brought out the best in Yuzna and frequent collaborator Stuart Gordon (also of HONEY, I SHRUNK THE KIDS fame...among other things), but it's interesting to see how they operate apart, to understand the unique ingredients that each filmmaker brought to the more perfect union of their classic Lovecraft adaptation. Gordon skewed darker and more intellectual, as evidenced by the end of his career with the shattering mob thriller KING OF THE ANTS, the disturbing true crime drama STUCK, and the Mamet-penned EDMOND. Yuzna, for his part, is almost anti-intellectual, preferring to cook up blackly comic, semi-pornographic nightmares like his two increasingly horny RE-ANIMATOR sequels, the terminal S&M fantasy RETURN OF THE LIVING DEAD 3, and the shamelessly hokey comic book adaptation FAUST: LOVE OF THE DAMNED. Yuzna's lack of shame is really his defining feature as an artist, and nowhere is this more obvious than in his directorial debut and signature masterpiece, SOCIETY.
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Salvador Dali's "The Great Masturbator," a chief visual inspiration for SOCIETY.
Yuzna was able to leverage the success of RE-ANIMATOR to lock in two directorial opportunities, BRIDE OF RE-ANIMATOR, and a bizarre body horror exercise about a Beverly Hills orphan who discovers that not only are his adoptive family from a different bloodline, but they're not even from the same species. That both pictures employed the writing team of Woody Keith and Rick Fry gives you a little taste of what to expect from SOCIETY, but to be frank, the latter threatens to make the former look like a very special episode of ER; "overkill" barely begins to describe SOCIETY’s ambitious assault on the human body. In a recent interview, the philipino-american director giggles perversely, "I think my friends were a little embarrassed for me (when they saw SOCIETY)," and this sound bite reminded me that the last, most important ingredient that Yuzna contributes to any project is unabashed joy. It's a little hard to imagine stomaching SOCIETY without it.
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In this unusual scene from the class struggle in Beverly Hills, Billy Warlock (son of HALLOWEEN 2's Michael Myers, Dick Warlock) plays Bill Whitney, a rich, handsome, athletic high school student with a heavy duty anxiety disorder. Although he appears to have it all, he is plagued by nightmares and hallucinations, reflecting suspicions that the family that spoils him is also out to get him. Perhaps this is all understandable, though. Bill is under a lot of pressure these days, with his parents devoting all of their attention to his sister's coming out party, and his narcissistic girlfriend pushing him to ingratiate himself to the assholes higher up the social ladder; it's enough to make any teenager feel alienated and insecure. But, do these garden variety anxieties account for his visions of his sister's body deforming itself unnaturally, or the dubious evidence he finds that her debutante ball involves incestuous orgies and human sacrifice? Is Bill simply crumbling under the strain of societal expectations, or is the friction with his shrink, his parents, and his peers all symptomatic of an elaborate plot against him by elites who are truly less than human?
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I can’t believe they use this cheapo blanket trick MORE THAN ONCE in a movie that is famous for its unforgettable special effects, and I guess I kind of love it.
In case I haven't made the answer abundantly obvious, I'll add that while SOCIETY is the purest expression of Yuzna-ness on the market, it has an important co-author in Screaming Mad George. The eccentric japanese FX master, whose name is apparently an amalgamation of Mad Magazine, Screamin' Jay Hawkins, and...George, has produced some of horror's most outrageous makeup and visual effects, mostly for Yuzna, many of them in SOCIETY. If you've seen even a trailer for Alex Winter's 1993 oddity FREAKED--which is itself a grossout criticism of American social standards--then you are already familiar with SMG's trademark style. He specializes in twisted perversions of the human form that would make a cenobite blush, driven by a penchant for puns, and influenced equally by THE THING's Rob Botin, and Big Daddy Roth’s Rat Fink style. Screaming Mad George is instrumental in articulating Yuzna's premise: that behind the shimmering veneer of success and sophistication, the upper class are just a bunch of degenerates, who literally degenerate into something unimaginable behind closed doors. It's impossible to imagine SOCIETY without his sinuous, slithering monstrosities, or his indescribable realization of their most important social event, "the shunt".
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One of many great images from a zine I wish I owned, on SMG’s Facebook page.
It's easy to get overwhelmed by SOCIETY's visual impact, but its message is just as potent now as it was at the end of the Reagan era: Rich people are not only different from the rest of us, but in fact, they aren't even human. Writers Keith and Fry make an interesting choice of hero to help put this across. A lazier writer would have selected any archetype from the Freaks and Geeks set to create an easy Us vs Them tension, but SOCIETY is led by a promising young man who, for reasons he himself does not yet understand, is just not "the right kind of people". Bill appears to have every advantage in life, including a level of popularity that wins him presidency of the debate team despite his nerdier rival’s superior prowess--and yet, he suffers from a stigmatizing psychiatric disorder that is the natural result of feeling indefinably different from one's peers, and intuiting that, as a consequence, they don't even really like you. The shallow jock with deep-seated emotional problems is a much more interesting protagonist for this kind of social allegory than the charismatic outcasts that you get in movies like THE FACULTY and DISTURBING BEHAVIOR, for whom the idea that the elites could be aliens is just de rigueur.
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It's worth noting that this complexity of character extends to Bill's love interest, sympathetic society girl Clarissa Carlyn (Playboy Playmate Devin DeVasquez). At first, she seems villainously eager to introduce Bill to the many splendors of "the shunting", but as the plot against him mounts to its horrifying conclusion, she defects. There appears to be a reason for this, although honestly, this is the most difficult part of SOCIETY for me to wrap my head around. Clarissa lives as an essentially independent adult, only burdened by her mother (Pamela Matheson), a possibly brain damaged hulk who lurks in and out of various scenes just to be disturbing, always announced by some toots on a tuba, before eventually siding with our heroes. I'm really not sure what's supposed to be going on in this part of the movie, except that this character contributes to a number of distasteful jokes. But, I hold on to the idea that by virtue of whatever disorder Mrs. Carlyn suffers from, she serves the purpose of priming Clarissa to rebel, since her very existence makes her daughter something of a societal outcast herself. That's the best I can do.
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In any case, everyone working on SOCIETY commits completely, with Mrs. Carlyn being no exception. The movie's climactic orgy of the damned is an all hands on deck operation, just as reliant on Screaming Mad George's artistic abilities as it is on the actors' responsibility to make you believe that this fucked up shit is really happening. There's a visceral patina of sleaze spread over the entire film, dripping from the way that characters talk to and touch each other, flirting and flaunting their bodies in a distinctly unseemly fashion, even when it stays within the realm of mundane reality. This constant sinister, insinuating attitude on the part of the whole cast lays the foundation for what is to come, and while I appreciate everybody's hard work, my favorite performance is from an actor who only comes in at the very end: David Wiley as society king Judge Carter. Wiley's career consisted almost exclusively of the most ordinary sort of television work, which makes his outrageous turn in this alien porno flick all the more respectable. While other characters transition from suspicious pod people to full-on mutated perverts, Judge Carter has to show up just for the finale, establish his authority, rip off his clothes, and plunge straight into a sea of slime, happily fisting his way through the cast. Wiley meets this challenge with aplomb, making of himself a hybrid of Robert Englund and Gene Hackman, perfectly embodying the movie's joyful absurdity, and never betraying the slightest hint of embarrassment. 
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SOCIETY is very much a don't-look-down type of endeavor, a fairy that could expire at the slightest lapse in faith. There's a visual pun in the last act that's so gross, so offensive, so frankly idiotic, that I don't have the courage to describe it; my whole body tenses up when I know this scene is coming, as if it were the meat hook scene in TEXAS CHAIN SAW MASSACRE or the brutal rape in the middle of SHOWGIRLS. I don't like it, but at the same time, I respect Yuzna's unhesitating commitment to show it to me, and I think that actor Charles Lucia should get some kind of award for shouldering the burden so valiantly. SOCIETY is a daring movie in the truest sense, a film with more balls than brains, and in this it exposes the limitation of intelligence and taste, and the real need for pure transgression, in producing art of any real value. You might argue with me about whether Yuzna's masturbatory magnum opus really qualifies as art, but to respond to that, I'll quote the great transgressor Alejandro Jodorowsky: "If you are great, EL TOPO is a great picture. If you are limited, EL TOPO is limited." So stick that in your shunt and smoke it.
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PS Here, have this stuck in your head for the rest of your life.
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scifigeneration · 5 years
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Einstein's general relativity theory is questioned but still stands for now
More than 100 years after Albert Einstein published his iconic theory of general relativity, it is beginning to fray at the edges, said Andrea Ghez, UCLA professor of physics and astronomy. Now, in the most comprehensive test of general relativity near the monstrous black hole at the center of our galaxy, Ghez and her research team report July 25 in the journal Science that Einstein's theory of general relativity holds up.
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"Einstein's right, at least for now," said Ghez, a co-lead author of the research. "We can absolutely rule out Newton's law of gravity. Our observations are consistent with Einstein's theory of general relativity. However, his theory is definitely showing vulnerability. It cannot fully explain gravity inside a black hole, and at some point we will need to move beyond Einstein's theory to a more comprehensive theory of gravity that explains what a black hole is."
Einstein's 1915 theory of general relativity holds that what we perceive as the force of gravity arises from the curvature of space and time. The scientist proposed that objects such as the sun and the Earth change this geometry. Einstein's theory is the best description of how gravity works, said Ghez, whose UCLA-led team of astronomers has made direct measurements of the phenomenon near a supermassive black hole -- research Ghez describes as "extreme astrophysics."
The laws of physics, including gravity, should be valid everywhere in the universe, said Ghez, who added that her research team is one of only two groups in the world to watch a star known as S0-2 make a complete orbit in three dimensions around the supermassive black hole at the center of the Milky Way. The full orbit takes 16 years, and the black hole's mass is about four million times that of the sun.
The researchers say their work is the most detailed study ever conducted into the supermassive black hole and Einstein's theory of general relativity.
The key data in the research were spectra that Ghez's team analyzed this April, May and September as her "favorite star" made its closest approach to the enormous black hole. Spectra, which Ghez described as the "rainbow of light" from stars, show the intensity of light and offer important information about the star from which the light travels. Spectra also show the composition of the star. These data were combined with measurements Ghez and her team have made over the last 24 years.
Spectra -- collected at the W.M. Keck Observatory in Hawaii using a spectrograph built at UCLA by a team led by colleague James Larkin -- provide the third dimension, revealing the star's motion at a level of precision not previously attained. (Images of the star the researchers took at the Keck Observatory provide the two other dimensions.) Larkin's instrument takes light from a star and disperses it, similar to the way raindrops disperse light from the sun to create a rainbow, Ghez said.
"What's so special about S0-2 is we have its complete orbit in three dimensions," said Ghez, who holds the Lauren B. Leichtman and Arthur E. Levine Chair in Astrophysics. "That's what gives us the entry ticket into the tests of general relativity. We asked how gravity behaves near a supermassive black hole and whether Einstein's theory is telling us the full story. Seeing stars go through their complete orbit provides the first opportunity to test fundamental physics using the motions of these stars."
Ghez's research team was able to see the co-mingling of space and time near the supermassive black hole. "In Newton's version of gravity, space and time are separate, and do not co-mingle; under Einstein, they get completely co-mingled near a black hole," she said.
"Making a measurement of such fundamental importance has required years of patient observing, enabled by state-of-the-art technology," said Richard Green, director of the National Science Foundation's division of astronomical sciences. For more than two decades, the division has supported Ghez, along with several of the technical elements critical to the research team's discovery. "Through their rigorous efforts, Ghez and her collaborators have produced a high-significance validation of Einstein's idea about strong gravity."
Keck Observatory Director Hilton Lewis called Ghez "one of our most passionate and tenacious Keck users." "Her latest groundbreaking research," he said, "is the culmination of unwavering commitment over the past two decades to unlock the mysteries of the supermassive black hole at the center of our Milky Way galaxy."
The researchers studied photons -- particles of light -- as they traveled from S0-2 to Earth. S0-2 moves around the black hole at blistering speeds of more than 16 million miles per hour at its closest approach. Einstein had reported that in this region close to the black hole, photons have to do extra work. Their wavelength as they leave the star depends not only on how fast the star is moving, but also on how much energy the photons expend to escape the black hole's powerful gravitational field. Near a black hole, gravity is much stronger than on Earth.
Ghez was given the opportunity to present partial data last summer, but chose not to so that her team could thoroughly analyze the data first. "We're learning how gravity works. It's one of four fundamental forces and the one we have tested the least," she said. "There are many regions where we just haven't asked, how does gravity work here? It's easy to be overconfident and there are many ways to misinterpret the data, many ways that small errors can accumulate into significant mistakes, which is why we did not rush our analysis."
Ghez, a 2008 recipient of the MacArthur "Genius" Fellowship, studies more than 3,000 stars that orbit the supermassive black hole. Hundreds of them are young, she said, in a region where astronomers did not expect to see them.
It takes 26,000 years for the photons from S0-2 to reach Earth. "We're so excited, and have been preparing for years to make these measurements," said Ghez, who directs the UCLA Galactic Center Group. "For us, it's visceral, it's now -- but it actually happened 26,000 years ago!"
This is the first of many tests of general relativity Ghez's research team will conduct on stars near the supermassive black hole. Among the stars that most interest her is S0-102, which has the shortest orbit, taking 11 1/2 years to complete a full orbit around the black hole. Most of the stars Ghez studies have orbits of much longer than a human lifespan.
Ghez's team took measurements about every four nights during crucial periods in 2018 using the Keck Observatory -- which sits atop Hawaii's dormant Mauna Kea volcano and houses one of the world's largest and premier optical and infrared telescopes. Measurements are also taken with an optical-infrared telescope at Gemini Observatory and Subaru Telescope, also in Hawaii. She and her team have used these telescopes both on site in Hawaii and remotely from an observation room in UCLA's department of physics and astronomy.
Black holes have such high density that nothing can escape their gravitational pull, not even light. (They cannot be seen directly, but their influence on nearby stars is visible and provides a signature. Once something crosses the "event horizon" of a black hole, it will not be able to escape. However, the star S0-2 is still rather far from the event horizon, even at its closest approach, so its photons do not get pulled in.)
Ghez's co-authors include Tuan Do, lead author of the Sciencepaper, a UCLA research scientist and deputy director of the UCLA Galactic Center Group; Aurelien Hees, a former UCLA postdoctoral scholar, now a researcher at the Paris Observatory; Mark Morris, UCLA professor of physics and astronomy; Eric Becklin, UCLA professor emeritus of physics and astronomy; Smadar Naoz, UCLA assistant professor of physics and astronomy; Jessica Lu, a former UCLA graduate student who is now a UC Berkeley assistant professor of astronomy; UCLA graduate student Devin Chu; Greg Martinez, UCLA project scientist; Shoko Sakai, a UCLA research scientist; Shogo Nishiyama, associate professor with Japan's Miyagi University of Education; and Rainer Schoedel, a researcher with Spain's Instituto de Astrofsica de Andalucia.
The National Science Foundation has funded Ghez's research for the last 25 years. More recently, her research has also been supported by the W.M. Keck Foundation, the Gordon and Betty Moore Foundation and the Heising-Simons Foundation.
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halloweendailynews · 6 years
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The Year of The Shape continues, as a group of indie filmmakers who share a love for Halloween have teamed up to faithfully recreate four iconic scenes from John Carpenter’s 1978 classic, along with fifth scene of their own, to be released online for free this month as part of the ongoing 40th anniversary celebration.
Halloween Daily News caught up with the fan film’s co-directors Michael T. Lombardi (who also portrays The Shape) and Nils Toledo Jr. to get the scoop on this project, which used look-like actors and tried to match costumes, settings. lighting, and camera angles as close as possible to how Carpenter did it. We asked them about what the original Halloween means to them, what inspired them to take on this experiment, and the challenges it presented. Read on for their answers, as well as a teaser trailer and some pretty impressive promo photos.
Why did you decide to undertake this shot-for-shot recreation?
Lombardi: I’m always looking for new challenges as a film maker and actor. When I saw all the excitement surrounding the 40th anniversary of Halloween and the upcoming release of David Gordon Green’s 2018 sequel, I knew I wanted to somehow be a part of that. Since I and my production team are big fans of the original film and have been influenced by the film making style of John Carpenter, we decided to attempt to faithfully recreate several iconic scenes from the original film.
To say that this is not an easy task is an understatement, but we were intrigued by the idea and definitely always love a challenge! We are acutely aware that Halloween fans are intensely passionate and notoriously hard to please, but we are Halloween fans too, and we saw this as an opportunity to have a lot of fun honoring a movie we love so much. And let me tell you, we had a lot of fun.
In my career, I’ve produced only original films and television projects, which is how it should be for any artist. I’ve watched countless Halloween fan films over the years, all of which took their cues directly from the original source material. In 2012, I produced a four-episode limited event series called Haddonfield Hills, which was my own interpretation of the Halloween story. We had a lot of fun with that, and it had a modest online following. But this shot-for-shot project is very different.
Toledo: We’re all fans of the original movie, and it’s the one movie that we all wanted to recreate. It was groundbreaking for its time and continues to be.
What does the original Halloween mean to you?
Lombardi: As a kid, I was easily scared and did not fully see the appeal of horror films, but I eventually came to appreciate the genre in all its forms. Halloween was the first horror film I ever watched, and it left its mark on me. The film was produced with such a high level of artistry and craftsmanship, and did so much, with so little. I’m not a fan of horror films that emphasize gore over scares, so the fact that Halloween has virtually no blood in it was very appealing to me. It proved that less is more.
The mask was simple but terrifying. The attention to detail with lighting and camera movements was revolutionary. I also really liked that the film had a strong, intelligent female protagonist at its core, which most horror films still lack even to this day. But it was Carpenter’s iconic music score that really affected me. It was haunting – and still is – no matter how many times I hear it. For me, Halloween is as perfect as a horror film gets.
Toledo: It’s the first movie I remember from childhood. My parents allowed me to see the movie very young (they were big horror fans) and it became the family go-to movie not only every Halloween, but we would watch it throughout the year. We were all enthralled in the fandom, the characters, the story, and mythology behind it.
What were the challenges you faced doing the shot-for-shot recreation?
Lombardi: The first challenge was casting. Not only did we need to find actors who were strong performers, but they also had to resemble the original actors as closely as possible. That being said, I think we got very lucky in both departments.
The next challenge was the locations. Early on in the scouting process, we gave up on being able to find homes here in Connecticut that matched the look of the houses that Carpenter used in Pasadena, California. That just wasn’t going to happen.  Interior wise, we had the same challenges, especially since this is a late ’70s period piece. Unless we built replica sets on a sound stage (and we didn’t have the budget for that), we were never going to match that look perfectly. What we did do was find locations that we felt allowed us to capture the same basic aesthetic as the original, and we then focused on duplicating the camera angles and lighting.
When people watch this, they may see that not every angle is exactly the same, or the lighting may be slightly different. We did have a few logistical challenges on-location, which were expected, and we did have to make compromises along the way. But I am very proud of what we were able to accomplish, and proud of our entire production team and cast. We can only hope that every Halloween fan out there who watches our little tribute will appreciate the incredible effort that went into this endeavor, and have as much fun viewing it as we did making it. This is an incredible year for Halloween!
Toledo: Originally, we wanted to exactly mimic this movie that we love so much. But since we had virtually no budget, you’re asking everybody to work for credit. The hurdle is to find actors and crew who are willing to work for free. The other thing is that we are attempting to recreate a movie which was shot on film, and employed a full production and lighting crew. We are shooting digital, utilizing modern-day lights, with a skeleton crew of five. We also had a challenge with shooting schedule, which was only four days.
The biggest narrative challenge we had was with the Annie Brackett scene. We wanted to shoot the laundry room scene, but we don’t have laundry rooms in a separate backyard location in Connecticut – that’s a California thing. So we had to get creative. Michael T. Lombardi was able to take that laundry scene, and two others featuring Annie (including her death scene in the car) and combine them into one big scene with some new, original dialogue, which allowed us to put our own unique spin on it. That was fun.
The official press release:
Michael T. Originals SHOT-FOR-SHOT in association with TNT Media presents John Carpenter’s “Halloween” will have its online premiere Friday, July 20, 2018. The independently shot “Halloween” tribute project is produced and directed by Michael T. Lombardi and Nils Toledo, Jr.
The short film project recreates four iconic scenes from John Carpenter’s 1978 horror film, with great care being taken to be as faithful to the original as possible. The production also recreated a fifth scene but put their own original spin on it. Local look-alike actors were cast, costumes were duplicated, and locations were chosen that allowed the filmmakers to capture the overall aesthetic of Carpenter’s classic. It should be noted that the production had virtually no budget, and was a true labor of love for all involved.
Lombardi and Toledo, themselves big fans of the original film, wanted to do something special to celebrate the 40th anniversary, and also to challenge themselves as filmmakers, with each scene being painstakingly shot to replicate the exact angles, lighting, and performances.
“As huge horror fans, the original ‘Halloween’ is our favorite film in the genre. It’s the perfect combination of great storytelling, solid production values, and an unforgettable performance by Jamie Lee Curtis. Our challenge has been to bring these five scenes back to life as accurately as possible and give the fans something to be excited about”, Lombardi said.
Prior to the premiere of the short film on July 20, “Halloween” fans can get a first look at the production with a Behind-the-Scenes “First Look” Special on Wednesday, July 11, 2018, which will include footage from the production and interviews with the cast and crew.
The cast includes Natalie Osborne as Laurie Strode, Emily Santarsiero as Annie Brackett, Patrick D’Andrea as Sam Loomis, Paul Noonan as Sheriff Leigh Brackett, Devin Murphy as Lindsey Wallace, Eli Wald as Tommy Doyle, and Michael T. Lombardi as The Shape, directed by Michael T. Lombardi (who is also Executive Producer) and Nils Toledo Jr. (who is also Director of Photography), and edited by Terese N. Toledo.
The short film can be viewed on the Michael T Originals YouTube Channel, Facebook, and other outlets.
#shotforshothalloween       #halloweenfanfilm2018
For more Halloween news, follow @HalloweenDaily.
Fans Recreated Iconic 'Halloween' Scenes Shot-for-Shot The Year of The Shape continues, as a group of indie filmmakers who share a love for…
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wsmith215 · 4 years
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2020 NFL offseason winners and losers
Let’s break down some of the winners and losers from this NFL offseason. Some of the stories in the short term were obvious — you don’t need me to tell you again who won the DeAndre Hopkins trade — but I’m going to try to take a look at the bigger picture to see how players, teams, coaches and others around the NFL were impacted by the moves and decisions made over the past few months.
Let’s start with a trio of young quarterbacks from the 2019 draft, all of whom are leaving the acquisition portion of the offseason as their teams’ starters. It begins with the player who might have the biggest shoes to fill of any player in NFL history:
Jump to a winner/loser: Clowney | Edwards-Helaire | Haskins Lock | Minshew | Murray | Newton Prescott | Rodgers | Stidham | Trubisky
Stidham is one of the most obvious victors of the past few months. We all knew the Patriots and Tom Brady would come to terms on a deal … until they didn’t. Then we all knew that the Pats were going to acquire Nick Foles or Andy Dalton or pull off some impossible run up the draft board for Tua Tagovailoa … and that didn’t happen either. Through the entire player acquisition window, the only competition the Patriots added for Stidham is veteran Brian Hoyer, who lost his last battle with Stidham for the backup spot in training camp in 2019. Barring a last-second move for Cam Newton, Stidham is going to be the Week 1 starter for the Patriots.
Merely having a chance to play is a huge opportunity for Stidham and one rarely afforded midround picks who aren’t forced into action by injury. Imagine if one of the other teams looking for quarterbacks in that draft range last year took Stidham instead? The Panthers paid Teddy Bridgewater in lieu of handing things over to Will Grier (pick No. 100). Ryan Finley (104) is buried behind first overall pick Joe Burrow in Cincinnati, while Easton Stick (166) is third behind Tyrod Taylor and sixth overall pick Justin Herbert in L.A. One other late-round selection will be starting in 2020 — see the next winner — but there are midround picks who don’t really get a chance to play meaningful football across their rookie deals. Stidham will get his.
Jarrett Stidham is taking over for Tom Brady in New England in 2020, and the Patriots are bringing back most of their offense. Rich Graessle/Icon Sportswire
The Patriots didn’t exactly add any star weapons for their new starter, but they did address their threadbare tight end room by using third-round picks on Devin Asiasi and Dalton Keene. Retaining guard Joe Thuney on a franchise tag and getting back center David Andrews from a pulmonary embolism means the Patriots should be well-positioned to protect Stidham. It’s obviously way too early to say anything about how he will perform, but he has gone from being an afterthought to taking the reins for Bill Belichick & Co.
Likewise, the Jaguars cleared out a path for their 2019 sixth-round pick, as they traded away free-agent addition Nick Foles after paying him more than $30 million for four starts. Jacksonville then sat out the various free-agent quarterback options and didn’t use either of its first-round picks on a signal-caller. The Jags even added Tyler Eifert at tight end and used a second-round pick on wideout Laviska Shenault Jr., though their desperate attempts to get anybody to take running back Leonard Fournette off their hands found no takers.
Again, even having a chance to take meaningful reps as a sixth-round pick is rare. The last sixth-rounder to throw at least 400 passes over his first two seasons was Tom Brady, who threw three as a rookie in 2000 and 413 while leading the Pats to a Super Bowl in 2001. Minshew is already way ahead of the game in terms of opportunity; now, with just Joshua Dobbs and sixth-round pick Jake Luton backing him up, Minshew should get a full season to prove he’s an NFL quarterback.
Let’s hit a 2019 quarterback trifecta! Lock flashed promise while going 4-1 across his five starts at the end of the season, though it’s worth noting that those four wins came against the teams ranked 20th (Chargers), 26th (Texans), 27th (Lions), and 30th (Raiders) in pass defense DVOA. At the very least, he did enough for the Broncos to feel confident about opening the 2020 season with him as their starter.
While Denver held out some hope for luring Tom Brady, it didn’t make a move for any of the other quarterbacks when Brady decided to stay east. The Broncos didn’t even bring in a significant backup — the depth chart behind Lock consists of Jeff Driskel, Brett Rypien and Riley Neal. This is Lock’s team.
Drew Lock had seven touchdown passes and three interceptions while playing the final five games for Denver. Tim Warner/Getty Images
On top of that vote of confidence from general manager John Elway, no quarterback gained more weapons this offseason than the Missouri product. Lock already had a handful of exciting pieces in running back Phillip Lindsay, wide receiver Courtland Sutton and tight end Noah Fant. I can’t pretend I’m the biggest Melvin Gordon fan, and it’s not a great contract for the Broncos, but the running back can be valuable when he’s healthy and protecting the football. Elway then used his first two selections in the draft on wideouts Jerry Jeudy and KJ Hamler.
Denver didn’t address its problematic left tackle spot, but it did make a major addition on the interior by signing lineman Graham Glasgow to a $44 million deal. The Broncos finished up by adding experienced offensive coordinator Pat Shurmur, who has gotten Sam Bradford, Case Keenum and Daniel Jones to exceed expectations over the past few seasons. It’s fair to be skeptical of Lock after just five starts, but outside of a left tackle, the 23-year-old has everything he could have asked for from his organization this offseason.
On the other hand, there’s a member of that 2019 quarterback class who might feel left out among all the additions. Washington did avoid the lure of using the second overall pick on a quarterback, but it did little to help its starting quarterback.
Haskins’ receiving corps beyond Terry McLaurin was lacking last season, and the most notable free agents his team imported to help out its young starter were Cody Latimer and Richard Rodgers. Washington used midround picks on hybrid back Antonio Gibson and wideout Antonio Gandy-Golden, but it also traded away star left tackle Trent Williams without adding a meaningful replacement.
Loser: Cam Newton, QB, free agent
Things haven’t worked out for the former league MVP, who might have hoped to play out the final year of his deal with the Panthers while earning $19.1 million. Newton was instead cut, and the coronavirus pandemic has prevented him from finding a new team. He hasn’t been able to conduct a public workout, though he has posted videos on Instagram that show him going through drills. In the meantime, the starting jobs and most of the prime backup jobs have been filled.
There are still at least seven teams that should be looking for a backup quarterback, including the aforementioned Broncos and Jaguars, who don’t seem to want to challenge their young starters. The Cardinals, Rams and Seahawks all need a veteran backup, but there’s little chance of Newton playing meaningful snaps for those teams in 2020.
2 Related
The two most logical landing spots left for Newton are in the AFC. Let’s start with the Titans, who gave Ryan Tannehill $91 million in practical guarantees over the next three years. Tannehill’s hold on the starting job isn’t going anywhere at that price tag, but the former Dolphins starter missed 24 games over his final four years in Miami. There’s a reasonable chance he misses time this year, and the Titans currently have seventh-round picks Cole McDonald and Logan Woodside behind their starter.
Tannehill was revelatory as a play-action passer last season, which fits what Newton does best. From 2017 through the first half of 2018, Newton posted a passer rating of 114.7 on play-action attempts, the seventh-best rate in the league. The Titans are built around Derrick Henry and their power-running attack, and it’s not difficult to imagine how Newton could play a role in that attack. A few starts for the Titans could help rebuild his value before the 2021 offseason.
The ideal job for Newton would be in Pittsburgh. The Steelers should get Ben Roethlisberger back after he missed 14 games in 2019 with an elbow injury, but the longtime starter is 38 and has missed 38 games over his 16-year career. Mason Rudolph and Devlin Hodges were replacement-level quarterbacks last season, and Newton could viably make his case to serve as Roethlisberger’s long-term replacement in Pittsburgh if he plays well in a couple of spot starts.
While the Bears started this offseason suggesting that Trubisky would be their Week 1 starter in 2020, their actions suggest that his future is tenuous. Chicago traded for Nick Foles, and in restructuring the former Super Bowl MVP’s deal, it guaranteed Foles $21 million over the next three seasons. Then the team declined Trubisky’s fifth-year option, which would have guaranteed a $24.8 million salary in 2021 for injury.
Failing to earn a fifth-year option pickup has typically been a bad sign. Eight other first-round quarterbacks have had their fifth-year option declined. None of them made it to a fifth year with the team that drafted them. Six of them — Jake Locker, EJ Manuel, Christian Ponder, Brandon Weeden, Johnny Manziel and Paxton Lynch — didn’t take an NFL snap anywhere in Year 5. Teddy Bridgewater spent his fifth year sitting behind Drew Brees, while the only one of the bunch who saw meaningful action was Blaine Gabbert in San Francisco.
Trubisky will instead have to look toward a teammate for hope. The Bears declined Kyle Fuller’s fifth-year option after injuries and inconsistent play, but after a breakout season, they used the transition tag to keep him around before matching a four-year, $56 million offer sheet. Fuller ended up making much more than he would have if the Bears had simply picked up that option in the first place. They have spent years trying to surround Trubisky with talent to confirm their belief that he was a franchise quarterback in the making. Now he has to overcome their skepticism and the odds.
There was little trade interest in Howard before he was dealt to the Eagles last offseason, and after seeing his rushing yards and yards-per-game figures decline in each of the past three seasons, I figured that the league would see him as a relatively replaceable zone runner. Alfred Morris, a similarly productive rookie, wasn’t able to ever get a significant deal.
Howard instead got a two-year, $10 million pact from the Dolphins with $4.8 million guaranteed in Year 1. Miami also added veterans Ereck Flowers and Ted Karras in free agency before using first- and second-round picks on offensive linemen. The Dolphins traded for Matt Breida, but they didn’t use a significant pick on a running back, and Breida has been a boom-or-bust player with injury issues during his time with the 49ers.
Howard landing meaningful guaranteed money, a starting job and a team that invested heavily in offensive linemen has to be considered a victory.
Jordan Howard averaged 4.4 yards per carry but only rushed 119 times for the Eagles last season. Eric Hartline/USA TODAY Sports
In a similar way to Newton’s, Clowney’s market has been depressed by medical concerns and an inability to evaluate those issues under the current climate. For all we hear about how NFL teams don’t focus on sacks, Clowney’s three-sack total from 2019 hasn’t helped his case. The former first overall pick is unquestionably talented, but the massive deal he might have received under typical circumstances after a more productive season hasn’t arrived.
Naturally, it seems like the logical thing for Clowney to do is sign a one-year deal with a contender and try to rebuild his value in the hopes of signing a big deal next year. Under normal circumstances, that idea makes sense. This isn’t a normal season, though, and there’s a chance that Clowney — and many other veterans — might not be able to sign big contracts next offseason.
As Jason Fitzgerald of Over the Cap wrote last week, the uncertainty around 2020 stadium and ticket revenue could lead to a meaningful drop in league income, which would result in a shrunken salary cap. Teams have seen the cap rise by an average of just under 6% over the past decade, up from $120 million in 2011 to $198.2 million in 2020. With players improving their share of revenue in the new CBA, the cap was expected to rise well north of $200 million in 2021. Now, Fitzgerald projects, the cap could fall somewhere between $130 million to $175 million in 2021, depending on how revenues are affected by the pandemic.
Obviously, it’s too early to project what the situation will be like next year, and the league could come to an agreement with its players to push future revenues forward to try to account for a reduced cap figure in 2021, but we could be looking at a different financial landscape next spring. Teams that were planning for a $210 million cap would be forced to cut veterans to get compliant, flooding the market with talented players. Many free agents would likely look for one-year deals in advance of a massive projected cap increase in 2022 and 2023, when local revenue would return to form and the league would be flush with television revenue from new deals. Clowney might end up stuck signing back-to-back one-year deals as a result.
Losers: Teams with lots of guaranteed money tied up in 2021
While we’re again months and months away from having any idea about what the cap will look like next year, there are teams that have to be sweating the possibility of a reduced cap. Take the Eagles, who already have $263.3 million on the books for 2021, much of it tied up in players who are core pieces of the roster. Getting down to $210 million would require a couple of restructures and cuts of veterans like DeSean Jackson, Alshon Jeffery and Marquise Goodwin. Moving to $175 million would require another $35 million in savings.
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The Eagles would find a reduced cap most difficult, but teams like the Saints, Falcons and Steelers would also be in compromised positions. Again, the league and players could come to terms on a deal that could restore some of the missing revenue, and the NFL would get a bump from a possible 17-game season in 2021, but the alternative looms as a dangerous scenario for several of the league’s highest-spending teams.
I hit the most crucial parts of the DeAndre Hopkins trade when it happened in March, but it’s quietly a huge victory for Johnson. With the Cardinals slapping the transition tag on Kenyan Drake, Arizona was clearly moving forward with Drake as its starting running back. It wouldn’t have been surprising to see Chase Edmonds as the No. 2 behind him. Johnson was likely in line to get cut, where veterans like Devonta Freeman, Carlos Hyde and LeSean McCoy haven’t found a market.
Instead, the Texans traded for Johnson as part of the Hopkins deal, suggesting that Bill O’Brien sees him as a meaningful asset. With Houston treating Duke Johnson like a third-down back last season, David Johnson has a clear path to lead-back duties in an offense that ranked 11th in rush offense DVOA a year ago. There’s even a chance that the Texans pay Johnson the $9 million he’s due in 2021, which seemed out of the question when the offseason began.
While I wrote about why the Jordan Love decision might not be as bad as it seems for the Packers, it’s fair to say that Rodgers’ position can’t feel as good as it did a few months ago.
Green Bay seemed to set a deadline on the Rodgers era, and the only shopping it did to help Rodgers this offseason was to swap out tight end Jimmy Graham for wide receiver Devin Funchess. I still think the Packers could go after a veteran wideout like Kenny Stills, but you can understand why Rodgers would be cranky right about now.
One year ago, the Rams were coming off a trip to the Super Bowl. Every team wanted to hire a coach who vaguely resembled Sean McVay. Their young core seemed set to compete for another title. After a frustrating 2019 campaign left the Rams struggling for answers on offense and out of the playoffs for the first time since McVay arrived in town, it was clear that Los Angeles needed to make changes during the offseason.
I’m not sure those changes really helped, as this offseason felt like a repudiation of the Rams’ philosophy. They lost legendary defensive coordinator Wade Phillips and longtime special-teams coordinator John Fassel. Just two years after handing out huge contracts to Brandin Cooks and Todd Gurley, they punted on both of those deals, cutting their former MVP candidate at running back while trading the wide receiver to the Texans. They were even publicly called out for not paying Gurley and Clay Matthews bonus money, which should hurt the organization when it tries to sign free agents in the future.
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Sean McVay says the Rams are fully focused on the Cowboys in Week 1 after the NFL schedule release.
Furthermore, the Rams didn’t really resolve any of their problems this offseason. After trading two first-round picks to acquire Jalen Ramsey, they still haven’t signed their star cornerback to an extension. They swapped out Dante Fowler Jr. for edge rusher Leonard Floyd and used their top two picks to replace Cooks and Gurley, but they didn’t do anything to replace star inside linebacker Cory Littleton.
Crucially, L.A. almost entirely ignored an offensive line that crumbled in 2019, re-signing aging left tackle Andrew Whitworth while choosing to hope for a healthier 2020. With Jared Goff posting the league’s worst passer rating under pressure in 2019, McVay will need to conjure up a solution to get his prize pupil back on track this season.
Well, duh. The Buccaneers have Tom Brady and Rob Gronkowski now. Even beyond those two additions, though, the offseason has gone extremely well for the Bucs. They needed to retain the core of their wildly underrated defensive line and managed to do so by franchising Shaq Barrett and re-signing both Jason Pierre-Paul and Ndamukong Suh. Their biggest hole heading into the draft was at right tackle, and they had to move up only one spot to get Tristan Wirfs.
This offseason was something out of a dream for Tampa Bay, which has a higher win projection in Vegas than the Patriots for 2020.
A particularly big winner in this scenario is Tampa Bay’s general manager. Licht has been the general manager for six years, and the Bucs have gone 34-62 during his time in charge. That’s the third-worst mark in football. The team has cycled through three coaches over that six-year span, and while Licht nailed first-round picks on wide receiver Mike Evans and defensive tackle Vita Vea, he’s also the one who drafted Jameis Winston and stuck with the embattled quarterback over the past five years. Licht also whiffed on most of his second-round selections, most notably kicker Roberto Aguayo, who was the low point of an almost comical inability from the organization to identify a competent kicker.
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Licht is by all accounts a nice guy, and he has hit on a number of his midround selections too. Teams are generally too aggressive in getting rid of their top decision-makers, and I’m not saying Licht should have been fired. Typically, though, general managers with that sort of track record don’t get to enter a seventh offseason, and when Licht did, he managed to convince Brady and Gronkowski to come to town. Nobody would have batted an eye if the Bucs let go of Licht last offseason; now, if the Bucs live up to expectations, he might very well win Executive of the Year.
Loser: Tight end streamers against the Arizona Cardinals
If you played daily fantasy football or chose to stream your tight ends on a week-to-week basis in standard fantasy football, you knew about the Cardinals. Last year, Arizona allowed 309 points to opposing tight ends in PPR leagues, an average of 19.3 points per game. No other team was above 244, and the league average was 195 points, or just under 12.2 points per contest. It’s the second-worst season any team has posted against tight ends over the past 20 years, trailing only the 2013 Cardinals. Everybody from T.J. Hockenson to Ross Dwelley had their best games of the season against Arizona.
Vance Joseph-led defenses don’t always know what to do with tight ends — the Broncos ranked 26th against tight ends during his two years as Denver’s coach — but the Cardinals did something to address the problem this offseason by drafting Isaiah Simmons with the No. 8 overall pick. They’ve suggested that the talented Clemson defender will begin his NFL career at linebacker, where he’s likely to see plenty of action against tight ends in coverage. Arizona has managed to get the least out of athletic, hybrid defenders like Deone Bucannon and Haason Reddick in years past, but Simmons could very well ruin one of the easiest exploits in fantasy football.
Did any first-round pick end up in a more advantageous landing spot? Andy Reid told general manager Brett Veach that he thought Edwards-Helaire was better than Brian Westbrook before the Chiefs drafted the LSU back with the final pick of the first round. The only running back Reid had drafted before the third round across his career as a head coach and personnel executive before Edwards-Helaire was LeSean McCoy, who was the 53rd pick in the 2009 draft.
While the Chiefs have suggested that Edwards-Helaire will split time with incumbent Damien Williams, the future belongs to the rookie. Williams is a free agent after the season and wasn’t healthy for most of 2019 with hamstring issues. The Chiefs also said the same thing about Kareem Hunt and Spencer Ware in 2017, and when Ware went down with a knee injury in the preseason, Hunt was handed the job and finished his rookie year with 1,782 yards from scrimmage. Edwards-Helaire should turn into one of the most productive backs in football; the only real question is when.
Losers: Rookie coaches (and players)
It should go without saying that this is incredibly low on the list of upheavals caused by the pandemic, but while the NFL has managed to keep free agency and the draft on schedule, there’s no realistic way for football teams to practice. With team facilities closed, organized team activities (OTAs) have been postponed and will likely be canceled. Rookie minicamps are being conducted remotely. It’s unclear whether teams will be able to undergo a full training camp.
As a result, newcomers seem likely to suffer. Some rookie players already have a difficult time catching up with the speed of the league and the complexity of professional playbooks; now they’ll have to try to catch up on the finer points over Zoom. Likewise, rookie coaches who are attempting to install a new scheme and work with new players already were going to have their practice time reduced over the summer by the new CBA. They’re almost surely going to miss out on any pre-training-camp practice time.
The Chargers took quarterback Justin Herbert at No. 6 overall, but Herbert likely won’t get many live reps in front of his coaches before training camp. Christian Petersen/Getty Images
Naturally, the teams with new head coaches and coordinators — the Browns, Giants, Panthers and Washington — are the ones that are most likely to suffer from this lack of teaching time. Teams with stability could benefit. In an indirect way, though they could not have possibly predicted what was going to happen, teams such as the Steelers and Texans who dealt away much of their draft capital could end up feeling better about their decisions, given that rookies may struggle to make an impact in 2020.
Winners: Veterans negotiating contracts with the Houston Texans
You probably knew that the Texans weren’t going to get out of a winners and losers column unscathed. I’ll leave the Hopkins deal aside, but it’s worth noting just how dramatically the contracts the Texans handed out differ from those of their peers. Slot corner Bradley Roby signed a three-year, $31.5 million deal when guys like Chris Harris Jr. and Brian Poole were forced to sign smaller contracts and Logan Ryan remains a free agent. Wideout Randall Cobb inked a three-year, $27 million deal when the wideout market totally cratered.
The biggest deal, though, belongs to Laremy Tunsil. The Texans didn’t sign the offensive tackle to an extension after trading two first-round picks and a second-rounder to the Dolphins last August. Tunsil said that even he would have made that trade from the Dolphins’ perspective, and he continued to dabble in negotiations when he chose to represent himself in extension talks with O’Brien.
Tunsil did well. He ended up signing a three-year, $66 million extension, meaning he’ll make a total of $76.9 million over the next four years. The deal shattered the tackle market, where the largest average annual salary belonged to Lane Johnson at $18 million per season, and Johnson’s deal is really a paper extension for cap purposes with base salaries that will void next offseason. The largest real deal for a tackle is Trent Brown’s four-year, $66.8 million pact from last offseason. Brown averaged less than $17 million per season on his deal. Tunsil averaged $22 million on his extension and $19.3 million over the next four years. Nobody in the league got a bigger contract this offseason after adjusting for positional expectations. Tunsil even gets to hit free agency again before turning 30. Not bad for a part-time agent!
I mentioned three other 2019 quarterbacks earlier, but I’ll add a fourth to the list with the first overall pick from last year’s draft. It isn’t complicated, of course: Murray was given the gift of DeAndre Hopkins, who will add to a receiving corps that already featured Christian Kirk and Larry Fitzgerald. The Arizona offense was also better after adding Kenyan Drake last season, and Drake was retained on a transition tag. Kliff Kingsbury’s offense will not lack for weapons.
I’m still a little worried about the offensive line, but the Cardinals did re-sign left tackle D.J. Humphries after his best season and added Josh Jones to compete with Marcus Gilbert on the right side. Last year’s MVP was a second-year quarterback who took a leap forward after his team spent the offseason surrounding him with the right weapons. It’s asking a lot of Murray to follow in the footsteps of Lamar Jackson, of course, but Murray should have the pieces he needs to take a leap forward in 2020.
I’ll finish up with one of the most interesting unresolved sagas of the offseason. No, Prescott doesn’t have his deal yet, though the star quarterback will have long-term financial security once he signs the $31.5 million franchise tag. The Cowboys continue to say they intend to keep Prescott around on a long-term deal, but they did add Andy Dalton and suggested last week that Prescott “has to accept what [the Cowboys] want to pay him.”
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Domonique Foxworth makes a case for why the Cowboys should sign Dak Prescott to a long-term contract.
Of course, Prescott doesn’t really have to accept that. The Cowboys can franchise him again in 2021 for $37.8 million, but with a third franchise tag costing them $54.3 million, they realistically have to get Prescott signed before the end of the 2021 season. And if the Cowboys think Prescott’s demands are unreasonable now, they’re not going to get cheaper, given that the likes of Deshaun Watson and Patrick Mahomes are going to raise the market by signing extensions of their own.
I’ve got a much bigger piece on the Prescott situation in the works, so I’m not going to get into the will they/should they questions here. What I will say, though, is that Prescott is in the catbird seat. The Cowboys let go of Jason Garrett, but they retained offensive coordinator Kellen Moore and star wide receiver Amari Cooper before adding another valuable weapon in rookie wideout CeeDee Lamb. Prescott lost veteran center Travis Frederick to retirement, but he’s well-positioned to deliver a big season for an offense that finished second in DVOA a year ago. If Prescott does that, well, the Cowboys might need to accept what Dak wants to be paid.
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The best available players after Round 1 of the 2020 NFL Draft
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Photograph by Ken Murray/Icon Sportswire via Getty Images
Houston offensive tackle Josh Jones highlights the best players for the second round on Friday.
In the end, after several twists, turns and false rumors, the beginning of the 2020 NFL Draft went as usual. And that goes beyond Joe Burrow going first and Chase Young going second. The Lions took cornerback Jeff Okudah at No. 3. The Giants took an offensive tackle. Tua Tagovailoa went to the Dolphins like most expected until people started assuming they would take Justin Herbert. The Chargers wisely took the best quarterback that fell to them in Herbert.
But not everything went according to plan. The wide receivers came off the board in an order few expected. Same for the offensive tackles. The first round was also filled with some stunners, like the Green Bay Packers moving up for quarterback Jordan Love or the Seattle Seahawks holding at No. 27 and taking linebacker Jordyn Brooks.
Those unexpected picks meant some big names fell out of the first round. Here are the best players available at the start of the second round of the 2020 NFL Draft, based on SB Nation’s top 100 players and then some:
21. Josh Jones, OT, Houston
22. A.J. Epenesa, Edge, Iowa
23. Grant Delpit, S, LSU
25. Yetur Gross-Matos, Edge, Penn State
26. Xavier McKinney, S, Alabama
27. Ezra Cleveland, OT, Boise State
28. Antoine Winfield Jr., S, Minnesota
31. Laviska Shenault Jr., WR, Colorado
32. D’Andre Swift, RB, Georgia
33. J.K. Dobbins, RB, Ohio State
34. Jonathan Greenard, Edge, Florida
35. Trevon Diggs, CB, Alabama
36. Denzel Mims, WR, Baylor
40. Ross Blacklock, DL, TCU
43. Jonathan Taylor, RB, Wisconsin
44. Tee Higgins, WR, Clemson
46. Michael Pittman Jr., WR, USC
47. Prince Tega Wanogho, OT, TCU
48. Jaylon Johnson, CB, Utah
49. Kristian Fulton, CB, LSU
50. Marlon Davidson, DL, Auburn
51. Curtis Weaver, Edge, Boise State
52. Lloyd Cushenberry, C, LSU
53. Justin Madubuike, DL, Texas A&M
54. Cameron Dantzler, CB, Mississippi State
56. KJ Hamler, WR, Penn State
57. Zack Baun, LB, Wisconsin
58. Kyle Dugger, S, Lenoir-Rhyne
59. Terrell Lewis, Edge, Alabama
60. Cam Akers, RB, Florida State
61. Julian Okwara, Edge, Notre Dame
62. Jeremy Chinn, S, Southern Illinois
63. Neville Gallimore, DL, Oklahoma
64. Robert Hunt, G, Louisiana
65. Matt Peart, OT, Connecticut
66. Josh Uche, Edge, Michigan
67. Bryan Edwards, WR, South Carolina
68. Van Jefferson, WR, Florida
69. Zack Moss, RB, Utah
70. Cole Kmet, TE, Notre Dame
71. Saahdiq Charles, OT, LSU
72. Jacob Eason, QB, Washington
73. Chase Claypool, WR, Notre Dame
74. Jabari Zuniga, Edge, Florida
75. Adam Trautman, TE, Dayton
76. Lucas Niang, OT, TCU
77. Jalen Hurts, QB, Oklahoma
78. Matt Hennessy, C, Temple
80. Jordan Elliott, DL, Missouri
81. Harrison Bryant, WR, Florida Atlantic
82. Alex Highsmith, Edge, Charlotte
83. Ashtyn Davis, S, California
84. Amik Robertson, CB, Louisiana Tech
85. Hunter Bryant, TE, Washington
86. Damien Lewis, G, LSU
87. James Lynch, DL, Baylor
89. Eno Benjamin, RB, Arizona State
90. Devin Duvernay, WR, Texas
91. Reggie Robinson, CB, Tulsa
92. Darrell Taylor, Edge, Tennessee
93. Akeem Davis-Gaither, LB, Appalachian State
94. Leki Fotu, DL, Utah
95. AJ Dillon, RB, Boston College
96. Khalid Kareem, Edge, Notre Dame
97. K’Von Wallace, S, Clemson
98. Willie Gay Jr., LB, Mississippi State
99. Colby Parkinson, TE, Stanford
100. Bradlee Anae, Edge, Utah
101. Jack Driscoll, OT, Auburn
102. Antonio Gibson, RB, Memphis
103. Lynn Bowden, WR/RB/QB, Kentucky
104. Alton Robinson, Edge, Syracuse
105. Raekwon Davis, DL, Alabama
106. Jonah Jackson, G, Ohio State
107. Tyler Biadasz, C, Wisconsin
108. Kenny Willekes, Edge, Michigan State
109. Jake Fromm, QB, Georgia
110. Gabriel Davis, WR, UCF
111. Netane Muti, G, Fresno State
112. Davon Hamilton, DL, Ohio State
113. Albert Okwuegbunam, TE, Missouri
114. Josiah Scott, CB, Michigan State
115. Collin Johnson, WR, Texas
116. Thaddeus Moss, TE, LSU
117. Troy Dye, LB, Oregon
118. Anfernee Jennings, Edge, Alabama
119. Antonio Gandy-Golden, WR, Liberty
120. Rashard Lawrence, DL, LSU
121. Trey Adams, OT, Washington
122. Jonathan Garvin, Edge, Miami
123. Nick Harris, C, Washington
124. Ke’Shawn Vaughn, RB, Vanderbilt
125. John Simpson, G, Clemson
126. Logan Wilson, LB, Wyoming
127. Ben Bartch, OT, Saint John’s (Minn.)
128. Kenny Robinson, S, West Virginia/XFL
129. John Hightower, WR, Boise State
130. Terrell Burgess, S, Utah
131. Devin Asiasi, TE, UCLA
132. Jason Strowbridge, DL, North Carolina
133. Alex Taylor, OT, South Carolina State
134. Logan Stenberg, G, Kentucky
135. Malik Harrison, LB, Ohio State
136. John Reid, CB, Penn State
137. Jared Pinkney, TE, Vanderbilt
138. Donovan Peoples-Jones, WR, Michigan
139. Lamar Jackson, CB, Nebraska
140. Joshua Kelley, RB, UCLA
141. Geno Stone, S, Iowa
142. Anthony Gordon, QB, Washington State
143. Tyler Johnson, WR, Minnesota
144. Anthony McFarland, RB, Maryland
145. Larrell Murchison, DL, North Carolina State
146. K.J. Hill, WR, Ohio State
147. A.J. Green, CB, Oklahoma State
148. Brandon Jones, S, Texas
149. Jauan Jennings, WR, Tennessee
150. Khalil Davis, DL, Nebraska
151. James Proche, WR, SMU
152. Bryce Hall, CB, Virginia
153. Markus Bailey, LB, Purdue
154. Calvin Throckmorton, OT, Oregon
155. Troy Pride Jr., CB, Notre Dame
156. Darryl Williams, C, Mississippi State
157. Benito Jones, DL, Ole Miss
158. Alohi Gillman, S, Notre Dame
159. Stanford Samuels III, CB, Florida State
160. Danny Pinter, G, Ball State
161. Derrek Tuszka, Edge, North Dakota State
162. Isaiah Hodgins, WR, Oregon State
163. Cole McDonald, QB, Hawaii
164. Joe Bachie, LB, Michigan State
165. Lavert Hill, CB, Michigan
166. Brycen Hopkins, TE, Purdue
167. J.R. Reed, S, Georgia
168. Quintez Cephus, WR, Wisconsin
169. McTelvin Agim, DL, Arkansas
170. Jacob Phillips, LB, LSU
171. Rodrigo Blankenship, K, Georgia
172. Darrynton Evans, RB, Appalachian State
173. Nate Stanley, QB, Iowa
174. Trajan Bandy, CB, Miami
175. D.J. Wonnum, Edge, South Carolina
176. Quartney Davis, WR, Texas A&M
177. Tanner Muse, S, Clemson
178. Davion Taylor, LB, Colorado
179. Solomon Kindley, G, Georgia
180. Stephen Sullivan, TE, LSU
181. Carlos Davis, DL, Nebraska
182. Essang Bassey, CB, Wake Forest
183. Kevin Dotson, G, Louisiana
184. Kalija Lipscomb, WR, Vanderbilt
185. Lamical Perine, RB, Florida
186. Carter Coughlin, Edge, Minnesota
187. Cam Brown, LB, Penn State
188. Levonta Taylor, S/CB, Florida State
189. Michael Onwenu, G, Michigan
190. Robert Landers, DL, Ohio State
191. David Woodward, LB, Utah State
192. Mason Fine, QB, North Texas
193. Trevis Gipson, Edge, Tulsa
194. Tyre Phillips, OT, Mississippi State
195. Michael Warren, RB, Cincinnati
196. Michael Ojemudia, CB, Iowa
197. Evan Weaver, LB, California
198. Jeff Thomas, WR, Miami
199. Nick Coe, Edge, Auburn
200. Dane Jackson, CB, Pittsburgh
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soxsick · 6 months
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studentsofshield · 7 years
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Monday Recs for May 15, 2017 - Nightwing aka Dick Grayson
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Following the retirement of his Robin persona, Dick Grayson became known as Nightwing. He emerged during the Judas Contract out from the shadow of Batman as his own man. After years of solo adventures, leading the Teen Titans, and the genesis of adulthood, it was time for Dick to graduate.
Fans know and love Dick Grayson as the optimist acrobat within the Batfamily. He also has quite the reputation as a superhero sex symbol, with his famous backside becoming its own industry meme. Whether he’s with Starfire, Barbara Gordon (the right one), or someone else, he’s also a ladies’ man. 
Dick has stepped into the Batman costume a few times and those stories are usually iconic, but he has decided he does not want to inherit that role. 
Most of Dick’s original Titans stories are written by Marv Wolfman. Many of his 1990s tales and the first 70 issues of his ongoing series were done by Chuck Dixon. Other writers like Devin Grayson and Peter Tomasi then left their mark on that title. 
Following Final Crisis and Grant Morrison’s Batman RIP storyline, the legendary writer put Dick in the boots and had him working alongside Damian Wayne as the new Robin. This was an intriguing role reversal with a bright and optimistic Batman with a brooding and aggressive Robin. Meanwhile, writers like Tony S. Daniel and Scott Snyder told the solo stories of Dick Grayson Batman.
The New 52 either hit Dick hard or not that bad, depends on who you ask. A decently received first ongoing by Kyle Higgins was soiled to many by a pointless costume change. Grayson then “died” in Forever Evil and got a costume-less spy-themed ongoing titled after his last name written by Tim Seeley and Tom King. In Rebirth, Tim Seeley is continuing on the character and getting fan approval with throwbacks to earlier eras using characters like Blockbuster and Professor Pyg.
Collection Information:
The Judas Contract has been collected several times throughout the years, with this being the most recent paperback version. For those trying to read all of New Teen Titans with Dick Grayson in it (previously as Robin), then this is the book to get. There is also a deluxe hardcover of the story coming soon, as well as omnibus volumes for NTT.
A Lonely Place of Dying is nowadays collected alongside A Death in the Family as one trade.
There is an old standalone trade just collecting Prodigal. The third volume of the most recent Knightfall reprints also includes it. Likewise the third omnibus of that arc contains it.
DC has been publishing a series of thick paperbacks recollecting Dick’s original solo series. -Volume 1: Bludhaven (Vol 1 1-4, Vol 2 1-8) -Rough Justice (9-18, Annual 1) -False Starts (19-25, Nightwing/Huntress 1-4) -Love and Bullets (26-34) -The Hunt for Oracle (35-46, Birds of Prey 20-21) -To Serve and Protect (47-53) -Shrike (54-60) More volumes are hopefully to come, at least through the end of Chuck Dixon’s run at 70. Or to 100 so that everything previously uncollected is covered.
Issues 101-153 of the first solo series have been collected in paperback before. Some are hard to track down now though.
Batman Era: -Battle for the Cowl -Batman and Robin: Batman Reborn (1-6) -Batman vs. Robin (7-12) -Batman and Robin Must Die (13-16) -The Black Mirror
There is an omnibus collecting all of the Grayson series. Otherwise it was collected in five thin volumes, since it was only 20 issues plus annuals/one-shots.
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tasksweekly · 7 years
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[TASK 045: FRECKLES]
There’s a masterlist below compiled of over 220+ faceclaims with freckles categorised by gender with their occupation and ethnicity denoted if there was a reliable source. If you want want an extra challenge use random.org to pick a random number! Of course everything listed below are just suggestions and you can pick whichever character or whichever project you desire.
Any questions can be sent here and all tutorials have been linked below the cut for ease of access! REMEMBER to tag your resources with #TASKSWEEKLY and we will reblog them onto the main! This task can be tagged with whatever you want but if you want us to see it please be sure that our tag is the first five tags!
THE TASK - scroll down for FC’s!
STEP 1: Decide on a FC you wish to create resources for! You can always do more than one but who are you starting with? There are links to masterlists you can use in order to find them and if you want help, just send us a message and we can pick one for you at random!
STEP 2: Pick what you want to create! You can obviously do more than one thing, but what do you want to start off with? Screencaps, RP icons, GIF packs, masterlists, PNG’s, fancasts, alternative FC’s - LITERALLY anything you desire!
STEP 3: Look back on tasks that we have created previously for tutorials on the thing you are creating unless you have whatever it is you are doing mastered - then of course feel free to just get on and do it. :)
STEP 4: Upload and tag with #TASKSWEEKLY! If you didn’t use your own screencaps/images make sure to credit where you got them from as we will not reblog packs which do not credit caps or original gifs from the original maker.
THINGS YOU CAN MAKE FOR THIS TASK -  examples are linked!
Stumped for ideas? Maybe make a masterlist or graphic of your favourite faceclaim with freckles. Plot ideas or screencaps from a music video preformed by a freckled artist. Masterlist of quotes and lyrics that can be used for starters, thread titles or tags.
Screencaps
RP icons [of all sizes]
Gif Pack [maybe gif icons if you wish]
PNG packs
Manips
Dash Icons
Character Aesthetics
PSD’s
XCF’s
Graphic Templates - can be chara header, promo, border or background PSD’s!
FC Masterlists - underused, with resources, without resources!
FC Help - could be related, family templates, alternatives.
Written Guides.
and whatever else you can think of / make!
MASTERLIST!
Note: If you’re using this masterlist for casting purposes please do further research before casting any of the following, it was difficult finding sources for most of these and don’t know if they’re ethnically or nationally Turkish. Many thanks.
We haven’t included those in THIS masterlist by @lazyresources so combined there are 220 facecalims!
Ladies:
Sissy Spacek (67) - actress and singer.
Dana Delany (61) - actress,, producer, presenter, and activist.
Sade (58) Nigerian (Yoruba), British - singer.
Mariska Hargitay (53) - actress.
Stacey Williams (49) - fashion model.
Alicia Coppola (49) - actress.
Jennifer Garner (45) - actress.
Julianne Nicholson (45) - actress.
Alyson Hannigan (43) - actress.
Neve Campbell (43) - actress.
Kate Moss (43) - model.
Amber Valletta (43) - model and actress.
Eva Longoria (42) Mexican (Spanish, Indigenous/Mayan, and African) - actress, producer, director, activist and businesswoman.
Kari Byron (42) - television host and artist.
Amy Smart (41) - actress and former fashion model.
Melissa Joan Hart (41) - actress, voice actress, director, producer, singer, fashion designer, and businesswoman.
Anna Friel (40) - actress.
Shakira (40) Lebanese / Colombian, including Italian/Sicilian, Spanish [Catalan, Castilian], possibly other - singer, songwriter, dancer, and record producer.
Jessica Chastain (40) - actress and film producer.
Annie Wersching (40) - actress.
Jennifer Hall (39) - actress.
Andrea Navedo (39) Puerto Rican - actress.
Jennifer Morrison (38) - actress, singer, producer, and director.
Angela Lindvall (38) - actress.
Michaela Maurerová (37) - actress.
Erin Cahill (37) - actress.
Vica Kerekes (36) - actress.
Gisele Bündchen (36) - model.
Bryce Dallas Howard (36) - actress, director, producer, and writer.
Meghan Markle (35) African-American / White -   actress, humanitarian, and activist.
Sienna Miller (35) - actress, model, and fashion designer.  
Diora Baird (34) - actress and former model.
Danielle Gamba (34) - model, dancer, and former NFL Cheerleader.
Natalie Britton (32) - actress.
Sarah Agor (32) - actress.
Anne Vyalitsyna (31) - model.
Michelle Trachtenberg (31) - actress.
Nicola Roberts (31) - recording artist, fashion designer, and songwriter.
Katrina Law (31) Taiwanese, German, Italian - actress.
Devin Kelley (31) - actress.
Caity Lotz (30) - actress, dancer, martial artist practitioner, singer, and model.
Katie Leclerc (30) - actress.
Kesha (30) - singer, songwriter, and rapper.
Virginia Petrucci (30) - actress.
Rose Leslie (30) 1/8th Mexican - actress.
Zoe Sloane (29) - actress.
Kristýna Kolocová (29) - beach volleyball player.
Blake Lively (29) - actress.
Karen Gillan (29) - actress and director.
Alia Shawkat (28) 50% Iraqi 25% Norwegian 12.5% Irish 12.5% Italian - actress.
Zoë Kravitz (28) 37.5% African-American 12.5% Afro-Bahamian 50% Ashkenazi Jewish - actress, singer, and model.
Gabriela Soukalová (27) - biathlete.
Adwoa Aboah (25) Ghanaian-British - model.
Binx Walton (21) Unknown Ethnicity - model.
Natalie Westling (20) - model.
Faye Reagan (?) - pornographic film actress.
Mia Sollis (?) - pornographic film actress.
JoJo (26) - singer, songwriter, and actress.
Meaghan Martin (25) - actress and singer.
Karle Warren (25) - actress.
Saoirse Ronan (23) - actress.
Laura Gwyneth Butler (born in 1997) - model.
Alexandra Porfirova (?) Unknown Ethnicity - model.
Jamillah McWhorter (?) Unknown Ethnicity - model.
Amit Freidman (?) - model.
Scarlett Fay (?) - pornographic film actress.
Adele Jacques (?) - actress.
Kim Blair (?) - actress.
Caroline Ford (?) - actress.
Ryann Shane (?) - actress.
Sarah Newswanger (?) - actress.
Juliet Oldfield (?) - actress.
Miyamoto Ayana (?) Japanese.
Males:
Damian Lewis (46) - actor.
David Tennant (46) - actor.
Jesse Williams (35) African-American, possibly Seminole Native American / White - actor, model, and activist.
Adam Wylie (33) - singer, musical performer, and voice actor.
Bob Morley (32) Filipino / White - actor.
Jay Hayden (30) - actor.
Higashide Masahiro (29) Japanese - actor and model.
Calum Worthy (26) - actor.
Diego Barrueco (26) - model.
Stephen Joffe (25) - actor.
Josh Hutcherson (24) - actor.
Adam Hicks (24) - actor, tapper, singer, and songwriter.
Adam Taylor Gordon (23) - actor.
Gabriel Basso (22) - actor.
Austin MacDonald (21) - actor.
Dylan Riley Snyder (20) - actor.
Zane Huett (20) - actor.
Dylan Minnette (20) - actor.
Jae Head (20) - actor.
Grayson Russell (19) - actor.
Justin Tinucci (18) - actor.
Elijah Nelson (18) - actor.
Tucker Albrizzi (17) - actor.
Shane Cambria (16) - actor.
George Hard (?) stated as biracial - model.
Johnny Harrington (?) - model.
Linus Wordemann (?) - model.
Kim Wonjung (?) Unknown Ethnicity - model.
Mat Lachance (?) - model.
Jester White (?) - model.
Devon Usher (?) - model.
Simonas Pham (?) Unknown Ethnicity - model.
Naleye Junior Dolmans (?) Unknown Ethnicity - model.
Jake Cassar (?) - model.
Tom Webb (?) - model.
Wynston Shannon (?) - model.
Calin Sitar (?) - model.
Victor Ross (?) Unknown Ethnicity - model.
Skyler James Sandak (?) - actor.
Bodhi Schulz (?) - actor.
Johannes Ibelherr (?) - model.
Peter Badenhop (?) - model.
Rodrigo Calazans (?) - model.
Adam Lee (?) - model.
Davi Vath (?) - model.
Florian Van Bael (?) - model.
Ismaelpeter Casillas Nelson (?) - actor.
Trans:
Buck Angel (44) film producer.
Taylor O'Keefe (?) - Youtuber.
Casil McArthur (?)
Use @ ur own discretion:
Eddie Redmayne
Emma Stone
Colton Haynes
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reneeacaseyfl · 5 years
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Detailed analysis of the star’s orbit near supermassive black hole gives a look into how gravity behaves — ScienceDaily
More than 100 years after Albert Einstein published his iconic theory of general relativity, it is beginning to fray at the edges, said Andrea Ghez, UCLA professor of physics and astronomy. Now, in the most comprehensive test of general relativity near the monstrous black hole at the center of our galaxy, Ghez and her research team report July 25 in the journal Science that Einstein’s theory of general relativity holds up.
“Einstein’s right, at least for now,” said Ghez, a co-lead author of the research. “We can absolutely rule out Newton’s law of gravity. Our observations are consistent with Einstein’s theory of general relativity. However, his theory is definitely showing vulnerability. It cannot fully explain gravity inside a black hole, and at some point we will need to move beyond Einstein’s theory to a more comprehensive theory of gravity that explains what a black hole is.”
Einstein’s 1915 theory of general relativity holds that what we perceive as the force of gravity arises from the curvature of space and time. The scientist proposed that objects such as the sun and the Earth change this geometry. Einstein’s theory is the best description of how gravity works, said Ghez, whose UCLA-led team of astronomers has made direct measurements of the phenomenon near a supermassive black hole — research Ghez describes as “extreme astrophysics.”
The laws of physics, including gravity, should be valid everywhere in the universe, said Ghez, who added that her research team is one of only two groups in the world to watch a star known as S0-2 make a complete orbit in three dimensions around the supermassive black hole at the center of the Milky Way. The full orbit takes 16 years, and the black hole’s mass is about four million times that of the sun.
The researchers say their work is the most detailed study ever conducted into the supermassive black hole and Einstein’s theory of general relativity.
The key data in the research were spectra that Ghez’s team analyzed this April, May and September as her “favorite star” made its closest approach to the enormous black hole. Spectra, which Ghez described as the “rainbow of light” from stars, show the intensity of light and offer important information about the star from which the light travels. Spectra also show the composition of the star. These data were combined with measurements Ghez and her team have made over the last 24 years.
Spectra — collected at the W.M. Keck Observatory in Hawaii using a spectrograph built at UCLA by a team led by colleague James Larkin — provide the third dimension, revealing the star’s motion at a level of precision not previously attained. (Images of the star the researchers took at the Keck Observatory provide the two other dimensions.) Larkin’s instrument takes light from a star and disperses it, similar to the way raindrops disperse light from the sun to create a rainbow, Ghez said.
“What’s so special about S0-2 is we have its complete orbit in three dimensions,” said Ghez, who holds the Lauren B. Leichtman and Arthur E. Levine Chair in Astrophysics. “That’s what gives us the entry ticket into the tests of general relativity. We asked how gravity behaves near a supermassive black hole and whether Einstein’s theory is telling us the full story. Seeing stars go through their complete orbit provides the first opportunity to test fundamental physics using the motions of these stars.”
Ghez’s research team was able to see the co-mingling of space and time near the supermassive black hole. “In Newton’s version of gravity, space and time are separate, and do not co-mingle; under Einstein, they get completely co-mingled near a black hole,” she said.
“Making a measurement of such fundamental importance has required years of patient observing, enabled by state-of-the-art technology,” said Richard Green, director of the National Science Foundation’s division of astronomical sciences. For more than two decades, the division has supported Ghez, along with several of the technical elements critical to the research team’s discovery. “Through their rigorous efforts, Ghez and her collaborators have produced a high-significance validation of Einstein’s idea about strong gravity.”
Keck Observatory Director Hilton Lewis called Ghez “one of our most passionate and tenacious Keck users.” “Her latest groundbreaking research,” he said, “is the culmination of unwavering commitment over the past two decades to unlock the mysteries of the supermassive black hole at the center of our Milky Way galaxy.”
The researchers studied photons — particles of light — as they traveled from S0-2 to Earth. S0-2 moves around the black hole at blistering speeds of more than 16 million miles per hour at its closest approach. Einstein had reported that in this region close to the black hole, photons have to do extra work. Their wavelength as they leave the star depends not only on how fast the star is moving, but also on how much energy the photons expend to escape the black hole’s powerful gravitational field. Near a black hole, gravity is much stronger than on Earth.
Ghez was given the opportunity to present partial data last summer, but chose not to so that her team could thoroughly analyze the data first. “We’re learning how gravity works. It’s one of four fundamental forces and the one we have tested the least,” she said. “There are many regions where we just haven’t asked, how does gravity work here? It’s easy to be overconfident and there are many ways to misinterpret the data, many ways that small errors can accumulate into significant mistakes, which is why we did not rush our analysis.”
Ghez, a 2008 recipient of the MacArthur “Genius” Fellowship, studies more than 3,000 stars that orbit the supermassive black hole. Hundreds of them are young, she said, in a region where astronomers did not expect to see them.
It takes 26,000 years for the photons from S0-2 to reach Earth. “We’re so excited, and have been preparing for years to make these measurements,” said Ghez, who directs the UCLA Galactic Center Group. “For us, it’s visceral, it’s now — but it actually happened 26,000 years ago!”
This is the first of many tests of general relativity Ghez’s research team will conduct on stars near the supermassive black hole. Among the stars that most interest her is S0-102, which has the shortest orbit, taking 11 ½ years to complete a full orbit around the black hole. Most of the stars Ghez studies have orbits of much longer than a human lifespan.
Ghez’s team took measurements about every four nights during crucial periods in 2018 using the Keck Observatory — which sits atop Hawaii’s dormant Mauna Kea volcano and houses one of the world’s largest and premier optical and infrared telescopes. Measurements are also taken with an optical-infrared telescope at Gemini Observatory and Subaru Telescope, also in Hawaii. She and her team have used these telescopes both on site in Hawaii and remotely from an observation room in UCLA’s department of physics and astronomy.
Black holes have such high density that nothing can escape their gravitational pull, not even light. (They cannot be seen directly, but their influence on nearby stars is visible and provides a signature. Once something crosses the “event horizon” of a black hole, it will not be able to escape. However, the star S0-2 is still rather far from the event horizon, even at its closest approach, so its photons do not get pulled in.)
Ghez’s co-authors include Tuan Do, lead author of the Science paper, a UCLA research scientist and deputy director of the UCLA Galactic Center Group; Aurelien Hees, a former UCLA postdoctoral scholar, now a researcher at the Paris Observatory; Mark Morris, UCLA professor of physics and astronomy; Eric Becklin, UCLA professor emeritus of physics and astronomy; Smadar Naoz, UCLA assistant professor of physics and astronomy; Jessica Lu, a former UCLA graduate student who is now a UC Berkeley assistant professor of astronomy; UCLA graduate student Devin Chu; Greg Martinez, UCLA project scientist; Shoko Sakai, a UCLA research scientist; Shogo Nishiyama, associate professor with Japan’s Miyagi University of Education; and Rainer Schoedel, a researcher with Spain’s Instituto de Astrofsica de Andalucia.
The National Science Foundation has funded Ghez’s research for the last 25 years. More recently, her research has also been supported by the W.M. Keck Foundation, the Gordon and Betty Moore Foundation and the Heising-Simons Foundation.
Credit: Source link
The post Detailed analysis of the star’s orbit near supermassive black hole gives a look into how gravity behaves — ScienceDaily appeared first on WeeklyReviewer.
from WeeklyReviewer https://weeklyreviewer.com/detailed-analysis-of-the-stars-orbit-near-supermassive-black-hole-gives-a-look-into-how-gravity-behaves-sciencedaily/?utm_source=rss&utm_medium=rss&utm_campaign=detailed-analysis-of-the-stars-orbit-near-supermassive-black-hole-gives-a-look-into-how-gravity-behaves-sciencedaily from WeeklyReviewer https://weeklyreviewer.tumblr.com/post/186550028602
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halloweendailynews · 7 years
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As we predicted, the highly anticipated new Halloween movie, to be executive produced by John Carpenter and arriving in theaters in October 2018, will ignore everything that happened in all of the franchise films after the original 1978 classic, according to recent statements from Carpenter himself.
In a new interview, John Carpenter tells Stereogum, “I may do the music for the new Halloween movie. That would be pretty easy to do… I’d like to do it. I’ve worked with them a little bit on the script. I’m just around to be a cheerleader for everybody.”
When asked about getting Jamie Lee Curtis back in the role of Laurie Strode, Carpenter says, “She talked to the director. Her part was written into the script and they had this idea — it’s kind of a… I don’t know how to describe it. It’s almost an alternative reality. It picks up after the first one and it pretends that none of the other [sequels] were made. It’s gonna be fun. There’s a really talented director and it was well-written. I’m impressed.”
I tweeted a few weeks ago that I think the new film will ignore everything after Part 1. Laurie is the new Loomis, claiming for 40 years He’s coming back. Then He does.
Judy Greer is currently in talks to play Karen Strode, who is Laurie Strode’s daughter in the new film.
As we recently reported, Halloween 2018 will begin filming at the end of October in Charleston, South Carolina.
Jamie Lee Curtis returns to her iconic role as Laurie Strode, who comes to her final confrontation with Michael Myers, the masked figure who has haunted her since she narrowly escaped his killing spree on Halloween night four decades ago.
Master of horror John Carpenter will executive produce and serve as creative consultant on this film, joining forces with cinema’s current leading producer of horror, Jason Blum (Get Out, Split, The Purge, Paranormal Activity). Inspired by Carpenter’s classic, filmmakers David Gordon Green and Danny McBride crafted a story that carves a new path from the events in the landmark 1978 film, and Green also directs.
HALLOWEEN will be produced by Malek Akkad, whose Trancas International Films has produced the HALLOWEEN series since its inception. Green and McBride will executive produce under their Rough House Pictures banner.
HALLOWEEN will be distributed worldwide by Universal Pictures.
David Gordon Green (Stronger, Our Brand Is Crisis, Joe, Pineapple Express) will direct the new Halloween from a screenplay by he and Danny McBride (Alien: Covenant, Eastbound & Down, Vice Principals).
John Carpenter will executive produce and may also score the film, with Malek Akkad producing for Trancas and Jason Blum producing for Blumhouse. Green and McBride will also executive produce under their Rough House Pictures banner. Zanne Devine and David Thwaites will oversee for Miramax, which is co-financing with Blumhouse.
You can read everything we know so far about Halloween 2018 here.
As I’m sure you are well aware, 2018 marks the 40th anniversary of the release of John Carpenter’s original 1978 Halloween. It is also worth noting that the film’s release date also happens to be Michael Myers’ birthday (in 1957), according to the original franchise canon.
The new Halloween arrives in theaters on October 19, 2018.
Keep watching this site for updates on the return of Michael Myers and all the latest news on the next Halloween movie!
I think the new film will ignore everything after Part 1. Laurie is the new Loomis, claiming for 40 years He’s coming back. Then He does.
— Halloween Daily News (@HalloweenDaily) September 17, 2017
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Jamie Lee Curtis returns as Laurie Strode in ‘Halloween’ 2018!
Read all of our HALLOWEEN 2018 coverage here!
For more Halloween news, follow @HalloweenDaily.
Happy #MichaelMyersMonday! John Carpenter Confirms 'Halloween' 2018 Ignores All Sequels (Told ya!) As we predicted, the highly anticipated new Halloween movie, to be executive produced by John Carpenter and arriving in theaters in October 2018, will ignore everything that happened in all of the franchise films after the original 1978 classic, according to recent statements from Carpenter himself.
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velmaemyers88 · 5 years
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Detailed analysis of the star’s orbit near supermassive black hole gives a look into how gravity behaves — ScienceDaily
More than 100 years after Albert Einstein published his iconic theory of general relativity, it is beginning to fray at the edges, said Andrea Ghez, UCLA professor of physics and astronomy. Now, in the most comprehensive test of general relativity near the monstrous black hole at the center of our galaxy, Ghez and her research team report July 25 in the journal Science that Einstein’s theory of general relativity holds up.
“Einstein’s right, at least for now,” said Ghez, a co-lead author of the research. “We can absolutely rule out Newton’s law of gravity. Our observations are consistent with Einstein’s theory of general relativity. However, his theory is definitely showing vulnerability. It cannot fully explain gravity inside a black hole, and at some point we will need to move beyond Einstein’s theory to a more comprehensive theory of gravity that explains what a black hole is.”
Einstein’s 1915 theory of general relativity holds that what we perceive as the force of gravity arises from the curvature of space and time. The scientist proposed that objects such as the sun and the Earth change this geometry. Einstein’s theory is the best description of how gravity works, said Ghez, whose UCLA-led team of astronomers has made direct measurements of the phenomenon near a supermassive black hole — research Ghez describes as “extreme astrophysics.”
The laws of physics, including gravity, should be valid everywhere in the universe, said Ghez, who added that her research team is one of only two groups in the world to watch a star known as S0-2 make a complete orbit in three dimensions around the supermassive black hole at the center of the Milky Way. The full orbit takes 16 years, and the black hole’s mass is about four million times that of the sun.
The researchers say their work is the most detailed study ever conducted into the supermassive black hole and Einstein’s theory of general relativity.
The key data in the research were spectra that Ghez’s team analyzed this April, May and September as her “favorite star” made its closest approach to the enormous black hole. Spectra, which Ghez described as the “rainbow of light” from stars, show the intensity of light and offer important information about the star from which the light travels. Spectra also show the composition of the star. These data were combined with measurements Ghez and her team have made over the last 24 years.
Spectra — collected at the W.M. Keck Observatory in Hawaii using a spectrograph built at UCLA by a team led by colleague James Larkin — provide the third dimension, revealing the star’s motion at a level of precision not previously attained. (Images of the star the researchers took at the Keck Observatory provide the two other dimensions.) Larkin’s instrument takes light from a star and disperses it, similar to the way raindrops disperse light from the sun to create a rainbow, Ghez said.
“What’s so special about S0-2 is we have its complete orbit in three dimensions,” said Ghez, who holds the Lauren B. Leichtman and Arthur E. Levine Chair in Astrophysics. “That’s what gives us the entry ticket into the tests of general relativity. We asked how gravity behaves near a supermassive black hole and whether Einstein’s theory is telling us the full story. Seeing stars go through their complete orbit provides the first opportunity to test fundamental physics using the motions of these stars.”
Ghez’s research team was able to see the co-mingling of space and time near the supermassive black hole. “In Newton’s version of gravity, space and time are separate, and do not co-mingle; under Einstein, they get completely co-mingled near a black hole,” she said.
“Making a measurement of such fundamental importance has required years of patient observing, enabled by state-of-the-art technology,” said Richard Green, director of the National Science Foundation’s division of astronomical sciences. For more than two decades, the division has supported Ghez, along with several of the technical elements critical to the research team’s discovery. “Through their rigorous efforts, Ghez and her collaborators have produced a high-significance validation of Einstein’s idea about strong gravity.”
Keck Observatory Director Hilton Lewis called Ghez “one of our most passionate and tenacious Keck users.” “Her latest groundbreaking research,” he said, “is the culmination of unwavering commitment over the past two decades to unlock the mysteries of the supermassive black hole at the center of our Milky Way galaxy.”
The researchers studied photons — particles of light — as they traveled from S0-2 to Earth. S0-2 moves around the black hole at blistering speeds of more than 16 million miles per hour at its closest approach. Einstein had reported that in this region close to the black hole, photons have to do extra work. Their wavelength as they leave the star depends not only on how fast the star is moving, but also on how much energy the photons expend to escape the black hole’s powerful gravitational field. Near a black hole, gravity is much stronger than on Earth.
Ghez was given the opportunity to present partial data last summer, but chose not to so that her team could thoroughly analyze the data first. “We’re learning how gravity works. It’s one of four fundamental forces and the one we have tested the least,” she said. “There are many regions where we just haven’t asked, how does gravity work here? It’s easy to be overconfident and there are many ways to misinterpret the data, many ways that small errors can accumulate into significant mistakes, which is why we did not rush our analysis.”
Ghez, a 2008 recipient of the MacArthur “Genius” Fellowship, studies more than 3,000 stars that orbit the supermassive black hole. Hundreds of them are young, she said, in a region where astronomers did not expect to see them.
It takes 26,000 years for the photons from S0-2 to reach Earth. “We’re so excited, and have been preparing for years to make these measurements,” said Ghez, who directs the UCLA Galactic Center Group. “For us, it’s visceral, it’s now — but it actually happened 26,000 years ago!”
This is the first of many tests of general relativity Ghez’s research team will conduct on stars near the supermassive black hole. Among the stars that most interest her is S0-102, which has the shortest orbit, taking 11 ½ years to complete a full orbit around the black hole. Most of the stars Ghez studies have orbits of much longer than a human lifespan.
Ghez’s team took measurements about every four nights during crucial periods in 2018 using the Keck Observatory — which sits atop Hawaii’s dormant Mauna Kea volcano and houses one of the world’s largest and premier optical and infrared telescopes. Measurements are also taken with an optical-infrared telescope at Gemini Observatory and Subaru Telescope, also in Hawaii. She and her team have used these telescopes both on site in Hawaii and remotely from an observation room in UCLA’s department of physics and astronomy.
Black holes have such high density that nothing can escape their gravitational pull, not even light. (They cannot be seen directly, but their influence on nearby stars is visible and provides a signature. Once something crosses the “event horizon” of a black hole, it will not be able to escape. However, the star S0-2 is still rather far from the event horizon, even at its closest approach, so its photons do not get pulled in.)
Ghez’s co-authors include Tuan Do, lead author of the Science paper, a UCLA research scientist and deputy director of the UCLA Galactic Center Group; Aurelien Hees, a former UCLA postdoctoral scholar, now a researcher at the Paris Observatory; Mark Morris, UCLA professor of physics and astronomy; Eric Becklin, UCLA professor emeritus of physics and astronomy; Smadar Naoz, UCLA assistant professor of physics and astronomy; Jessica Lu, a former UCLA graduate student who is now a UC Berkeley assistant professor of astronomy; UCLA graduate student Devin Chu; Greg Martinez, UCLA project scientist; Shoko Sakai, a UCLA research scientist; Shogo Nishiyama, associate professor with Japan’s Miyagi University of Education; and Rainer Schoedel, a researcher with Spain’s Instituto de Astrofsica de Andalucia.
The National Science Foundation has funded Ghez’s research for the last 25 years. More recently, her research has also been supported by the W.M. Keck Foundation, the Gordon and Betty Moore Foundation and the Heising-Simons Foundation.
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