THE EVE-ONLINE COMPENDIUM Compiled by Logixcraft
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Crossmedia Adaptation and the Development of Continuity in the Dc Animated Universe
“INFINITE EARTHS”: CROSSMEDIA ADAPTATION AND THE DEVELOPMENT OF CONTINUITY IN THE DC ANIMATED UNIVERSE Alex Nader A Thesis Submitted to the Graduate College of Bowling Green State University in partial fulfillment of the requirements for the degree of MASTER OF ARTS May 2015 Committee: Jeff Brown, Advisor Becca Cragin © 2015 Alexander Nader All Rights Reserved iii ABSTRACT Jeff Brown, Advisor This thesis examines the process of adapting comic book properties into other visual media. I focus on the DC Animated Universe, the popular adaptation of DC Comics characters and concepts into all-ages programming. This adapted universe started with Batman: The Animated Series and comprised several shows on multiple networks, all of which fit into a shared universe based on their comic book counterparts. The adaptation of these properties is heavily reliant to intertextuality across DC Comics media. The shared universe developed within the television medium acted as an early example of comic book media adapting the idea of shared universes, a process that has been replicated with extreme financial success by DC and Marvel (in various stages of fruition). I address the process of adapting DC Comics properties in television, dividing it into “strict” or “loose” adaptations, as well as derivative adaptations that add new material to the comic book canon. This process was initially slow, exploding after the first series (Batman: The Animated Series) changed networks and Saturday morning cartoons flourished, allowing for more opportunities for producers to create content. References, crossover episodes, and the later series Justice League Unlimited allowed producers to utilize this shared universe to develop otherwise impossible adaptations that often became lasting additions to DC Comics publishing. -
The Significance of Anime As a Novel Animation Form, Referencing Selected Works by Hayao Miyazaki, Satoshi Kon and Mamoru Oshii
The significance of anime as a novel animation form, referencing selected works by Hayao Miyazaki, Satoshi Kon and Mamoru Oshii Ywain Tomos submitted for the degree of Doctor of Philosophy Aberystwyth University Department of Theatre, Film and Television Studies, September 2013 DECLARATION This work has not previously been accepted in substance for any degree and is not being concurrently submitted in candidature for any degree. Signed………………………………………………………(candidate) Date …………………………………………………. STATEMENT 1 This dissertation is the result of my own independent work/investigation, except where otherwise stated. Other sources are acknowledged explicit references. A bibliography is appended. Signed………………………………………………………(candidate) Date …………………………………………………. STATEMENT 2 I hereby give consent for my dissertation, if accepted, to be available for photocopying and for inter-library loan, and for the title and summary to be made available to outside organisations. Signed………………………………………………………(candidate) Date …………………………………………………. 2 Acknowledgements I would to take this opportunity to sincerely thank my supervisors, Elin Haf Gruffydd Jones and Dr Dafydd Sills-Jones for all their help and support during this research study. Thanks are also due to my colleagues in the Department of Theatre, Film and Television Studies, Aberystwyth University for their friendship during my time at Aberystwyth. I would also like to thank Prof Josephine Berndt and Dr Sheuo Gan, Kyoto Seiko University, Kyoto for their valuable insights during my visit in 2011. In addition, I would like to express my thanks to the Coleg Cenedlaethol for the scholarship and the opportunity to develop research skills in the Welsh language. Finally I would like to thank my wife Tomoko for her support, patience and tolerance over the last four years – diolch o’r galon Tomoko, ありがとう 智子. -
Media Industry Approaches to Comic-To-Live-Action Adaptations and Race
From Serials to Blockbusters: Media Industry Approaches to Comic-to-Live-Action Adaptations and Race by Kathryn M. Frank A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy (Communication) in the University of Michigan 2015 Doctoral Committee: Associate Professor Amanda D. Lotz, Chair Professor Susan J. Douglas Professor Lisa A. Nakamura Associate Professor Aswin Punathambekar © Kathryn M. Frank 2015 “I don't remember when exactly I read my first comic book, but I do remember exactly how liberated and subversive I felt as a result.” ― Edward W. Said, Palestine For Mom and Dad, who taught me to be my own hero ii Acknowledgements There are so many people without whom this project would never have been possible. First and foremost, my parents, Paul and MaryAnn Frank, who never blinked when I told them I wanted to move half way across the country to read comic books for a living. Their unending support has taken many forms, from late-night pep talks and airport pick-ups to rides to Comic-Con at 3 am and listening to a comics nerd blather on for hours about why Man of Steel was so terrible. I could never hope to repay the patience, love, and trust they have given me throughout the years, but hopefully fewer midnight conversations about my dissertation will be a good start. Amanda Lotz has shown unwavering interest and support for me and for my work since before we were formally advisor and advisee, and her insight, feedback, and attention to detail kept me invested in my own work, even in times when my resolve to continue writing was flagging. -
Postfeminism in Female Team Superhero Comic Books by Showing the Opposite of The
POSTFEMINISM IN FEMALE TEAM SUPERHERO COMIC BOOKS by Elliott Alexander Sawyer A thesis submitted to the faculty of The University of Utah in partial fulfillment of the requirements for the degree of Master of Science Department of Communication The University of Utah August 2014 Copyright © Elliott Alexander Sawyer 2014 All Rights Reserved The University of Utah Graduate School STATEMENT OF THESIS APPROVAL The following faculty members served as the supervisory committee chair and members for the thesis of________Elliott Alexander Sawyer__________. Dates at right indicate the members’ approval of the thesis. __________Robin E. Jensen_________________, Chair ____5/5/2014____ Date Approved _________Sarah Projansky__________________, Member ____5/5/2014____ Date Approved _________Marouf Hasian, Jr.________________, Member ____5/5/2014____ Date Approved The thesis has also been approved by_____Kent A. Ono_______________________ Chair of the Department/School/College of_____Communication _______ and by David B. Kieda, Dean of The Graduate School. ABSTRACT Comic books are beginning to be recognized for their impact on society because they inform, channel, and critique cultural norms. This thesis investigates how comic books interact and forward postfeminism. Specifically, this thesis explores the ways postfeminism interjects itself into female superhero team comic books. These comics, with their rosters of only women, provide unique perspectives on how women are represented in comic books. Additionally, the comics give insight into how women bond with one another in a popular culture text. The comics critiqued herein focus on transferring postfeminist ideals in a team format to readers, where the possibilities for representing powerful connections between women are lost. Postfeminist characteristics of consumption, sexual freedom, and sexual objectification are forwarded in the comic books, while also promoting aspects of racism. -
“I Am the Villain of This Story!”: the Development of the Sympathetic Supervillain
“I Am The Villain of This Story!”: The Development of The Sympathetic Supervillain by Leah Rae Smith, B.A. A Thesis In English Submitted to the Graduate Faculty of Texas Tech University in Partial Fulfillment of the Requirements for the Degree of MASTER OF ARTS Approved Dr. Wyatt Phillips Chair of the Committee Dr. Fareed Ben-Youssef Mark Sheridan Dean of the Graduate School May, 2021 Copyright 2021, Leah Rae Smith Texas Tech University, Leah Rae Smith, May 2021 ACKNOWLEDGMENTS I would like to share my gratitude to Dr. Wyatt Phillips and Dr. Fareed Ben- Youssef for their tutelage and insight on this project. Without their dedication and patience, this paper would not have come to fruition. ii Texas Tech University, Leah Rae Smith, May 2021 TABLE OF CONTENTS ACKNOWLEDGMENTS………………………………………………………….ii ABSTRACT………………………………………………………………………...iv I: INTRODUCTION……………………………………………………………….1 II. “IT’S PERSONAL” (THE GOLDEN AGE)………………………………….19 III. “FUELED BY HATE” (THE SILVER AGE)………………………………31 IV. "I KNOW WHAT'S BEST" (THE BRONZE AND DARK AGES) . 42 V. "FORGIVENESS IS DIVINE" (THE MODERN AGE) …………………………………………………………………………..62 CONCLUSION ……………………………………………………………………76 BIBLIOGRAPHY …………………………………………………………………82 iii Texas Tech University, Leah Rae Smith, May 2021 ABSTRACT The superhero genre of comics began in the late 1930s, with the superhero growing to become a pop cultural icon and a multibillion-dollar industry encompassing comics, films, television, and merchandise among other media formats. Superman, Spider-Man, Wonder Woman, and their colleagues have become household names with a fanbase spanning multiple generations. However, while the genre is called “superhero”, these are not the only costume clad characters from this genre that have become a phenomenon. -
Line-Profile Variations of Stochastically Excited
A&A 515, A43 (2010) Astronomy DOI: 10.1051/0004-6361/200912777 & c ESO 2010 Astrophysics Line-profile variations of stochastically excited oscillations in four evolved stars S. Hekker1,2,3 and C. Aerts2,4 1 School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK e-mail: [email protected] 2 Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 D, 3001 Leuven, Belgium 3 Royal Observatory of Belgium, Ringlaan 3, 1180 Brussels, Belgium 4 Department of Astrophysics, IMAP, University of Nijmegen, PO Box 9010, 6500 GL Nijmegen, The Netherlands Received 29 June 2009 / Accepted 8 February 2010 ABSTRACT Context. Since solar-like oscillations were first detected in red-giant stars, the presence of non-radial oscillation modes has been de- bated. Spectroscopic line-profile analysis was used in the first attempt to perform mode identification, which revealed that non-radial modes are observable. Despite the fact that the presence of non-radial modes could be confirmed, the degree or azimuthal order could not be uniquely identified. Here we present an improvement to this first spectroscopic line-profile analysis. Aims. We aim to study line-profile variations in stochastically excited solar-like oscillations of four evolved stars to derive the az- imuthal order of the observed mode and the surface rotational frequency. Methods. Spectroscopic line-profile analysis is applied to cross-correlation functions, using the Fourier parameter fit method on the amplitude and phase distributions across the profiles. Results. For four evolved stars, β Hydri (G2IV), Ophiuchi (G9.5III), η Serpentis (K0III) and δ Eridani (K0IV) the line-profile vari- ations reveal the azimuthal order of the oscillations with an accuracy of ±1. -
Astronomy Magazine 2011 Index Subject Index
Astronomy Magazine 2011 Index Subject Index A AAVSO (American Association of Variable Star Observers), 6:18, 44–47, 7:58, 10:11 Abell 35 (Sharpless 2-313) (planetary nebula), 10:70 Abell 85 (supernova remnant), 8:70 Abell 1656 (Coma galaxy cluster), 11:56 Abell 1689 (galaxy cluster), 3:23 Abell 2218 (galaxy cluster), 11:68 Abell 2744 (Pandora's Cluster) (galaxy cluster), 10:20 Abell catalog planetary nebulae, 6:50–53 Acheron Fossae (feature on Mars), 11:36 Adirondack Astronomy Retreat, 5:16 Adobe Photoshop software, 6:64 AKATSUKI orbiter, 4:19 AL (Astronomical League), 7:17, 8:50–51 albedo, 8:12 Alexhelios (moon of 216 Kleopatra), 6:18 Altair (star), 9:15 amateur astronomy change in construction of portable telescopes, 1:70–73 discovery of asteroids, 12:56–60 ten tips for, 1:68–69 American Association of Variable Star Observers (AAVSO), 6:18, 44–47, 7:58, 10:11 American Astronomical Society decadal survey recommendations, 7:16 Lancelot M. Berkeley-New York Community Trust Prize for Meritorious Work in Astronomy, 3:19 Andromeda Galaxy (M31) image of, 11:26 stellar disks, 6:19 Antarctica, astronomical research in, 10:44–48 Antennae galaxies (NGC 4038 and NGC 4039), 11:32, 56 antimatter, 8:24–29 Antu Telescope, 11:37 APM 08279+5255 (quasar), 11:18 arcminutes, 10:51 arcseconds, 10:51 Arp 147 (galaxy pair), 6:19 Arp 188 (Tadpole Galaxy), 11:30 Arp 273 (galaxy pair), 11:65 Arp 299 (NGC 3690) (galaxy pair), 10:55–57 ARTEMIS spacecraft, 11:17 asteroid belt, origin of, 8:55 asteroids See also names of specific asteroids amateur discovery of, 12:62–63 -
Dissertation
Dissertation submitted to the Instituto de Astrofísica, Facultad de Física Pontificia Universidad Católica de Chile, Chile for the degree of Doctor in Astrophysics submitted to the Combined Faculties for the Natural Sciences and for Mathematics of the Ruperto-Carola University of Heidelberg, Germany for the degree of Doctor of Natural Sciences Put forward by M.Sc. Gergely Hajdu Born in Miskolc, Hungary Oral examination: 06 August 2019 Structure of the obscured Galactic disk with pulsating variables Gergely Hajdu Referees: Prof. Dr. Márcio Catelan Prof. Dr. Eva Grebel ABSTRACT Bright pulsating variables, such as Cepheids and RR Lyrae, are prime probes of the structure of both the young and old stellar components of the Milky Way. However, the far side of the Galactic disk has not yet been mapped using such variables as tracers, due to the severe extinction caused by foreground interstellar dust. In this thesis, the near-infrared light curves from the VISTA Variables in the Vía Láctea survey are utilized to penetrate these regions of high extinction and thus discover thou- sands of previously “hidden” Cepheid and RR Lyrae variables. The analysis of the light curves of RR Lyrae variables, was performed with a newly developed fitting algorithm, and their metallicities determined from their near-infrared light-curve shapes, using a newly developed method. These photometric metal abundances, combined with their positions within the Galactic disk, lend support to theories of an early, inside-out forma- tion of the Galactic disk. The newly discovered Cepheids were classified into the old (Type II) and young (Clas- sical) subtypes. A new near-infrared extinction law was determined using the Type II Cepheids, taking advantage of their concentration around the Galactic center. -
One of the Most Useful Accessories an Amateur Can Possess Is One of the Ubiquitous Optical Filters
One of the most useful accessories an amateur can possess is one of the ubiquitous optical filters. Having been accessible previously only to the professional astronomer, they came onto the marker relatively recently, and have made a very big impact. They are useful, but don't think they're the whole answer! They can be a mixed blessing. From reading some of the advertisements in astronomy magazines you would be correct in thinking that they will make hitherto faint and indistinct objects burst into vivid observ ability. They don't. What the manufacturers do not mention is that regardless of the filter used, you will still need dark and transparent skies for the use of the filter to be worthwhile. Don't make the mistake of thinking that using a filter from an urban location will always make objects become clearer. The first and most immediately apparent item on the downside is that in all cases the use of a filter reduces the amount oflight that reaches the eye, often quite sub stantially. The brightness of the field of view and the objects contained therein is reduced. However, what the filter does do is select specific wavelengths of light emitted by an object, which may be swamped by other wavelengths. It does this by suppressing the unwanted wavelengths. This is particularly effective in observing extended objects such as emission nebulae and planetary nebulae. In the former case, use a filter that transmits light around the wavelength of 653.2 nm, which is the spectral line of hydrogen alpha (Ha), and is the wavelength oflight respons ible for the spectacular red colour seen in photographs of emission nebulae. -
The 2020 Investor Day Programming Fact Sheet
THE 2020 INVESTOR DAY PROGRAMMING FACT SHEET ©Disney Today at The Walt Disney Company’s Investor Day event, Lucasfilm President Kathleen Kennedy announced an impressive number of exciting Disney+ series and new feature films destined to expand theStar Wars galaxy like never before. Introducing the Disney+ slate, Kennedy said, “We have a vast and expansive timeline in the Star Wars mythology spanning over 25,000 years of history in the galaxy—with each era being a rich resource for storytelling. Now with Disney+, we can explore limitless story possibilities like never before and fulfill the promise that there is truly a Star Wars story for everyone.” Among the 10 projects announced for Disney+ is “Obi-Wan Kenobi,” starring Ewan McGregor, with Hayden Christensen returning as Darth Vader, in what Kennedy called, “the rematch of the century.” Also announced are two new series from Jon Favreau and Dave Filoni, off-shoots of the multiple Emmy®-winning “The Mandalorian.” “Rangers of the New Republic” and “Ahsoka,” a series featuring the fan-favorite character Ahsoka Tano, will take place in “The Mandalorian” timeline. Kennedy announced that the next Star Wars feature film, releasing in December 2023, will be “Rogue Squadron,” which will be directed by Patty Jenkins of the “Wonder Woman” franchise. In July 2022, the next installment of the “Indiana Jones” franchise premieres, starring Harrison Ford, who reprises his iconic role. The film is directed by James Mangold. Following are the announced projects, listed in announcement order under the Disney+ and feature film headers: DISNEY+ Ahsoka After making her long-awaited, live-action debut in “The Mandalorian,” Ahsoka Tano’s story, written by Dave Filoni, will continue in a limited series, Ahsoka, starring Rosario Dawson and executive produced by Dave Filoni and Jon Favreau. -
A Special Case of an Error, in the Observed Time of a Star's Transit
3 200 On a small Nebula close to M. 57. By E. E. Barnard. In examining the annular Nebula of Lyra (M. 57) P with the 36 inch on October inld,I noticed a rather con- spicuous nebula in the field with it, and north preceding. As I have seen no record of this object, I have measured its position referred to the centre of the Ring Nebula, or rather with reference to the small star in the middle of the ring. 0 October and the da and dd were measured and October 8 the position angle and distance. ... Neb. - M. 57 ‘893 da Ad . oct 2 -20615 +131:1 -202.9 8 ____+ 133.3 -204.7 f132.2 The Aa and Ad for October 8, being derived from the following position angle and distance : P. A. = 303?3 Dist. = 2421’8 This nebula is about 1j2‘ diameter. Not round. A little brighter in the middle. About 14‘~magnitude. Inclosed is a sketch of its position (diam. of field a’&). I have not shown all the stars that are easily seen in this field. f Mt. Hamilton 1893 Oct. 8. E. E. Barnard. A Special Case of an Error, in the observed Time of a Star’s Transit, which is a Function of the Star’g Magnitude. By J. M. Schatberle. I In January 1891 I received a letter from Professor screens superposed reduced the brightness by about four Auwers of Berlin in which he informed me that from and six magnitudes respectively. a discussion of a series of observations sent to him it The program adopted was as follows. -
Stephen M. Cabrinety Collection in the History of Microcomputing, Ca
http://oac.cdlib.org/findaid/ark:/13030/kt529018f2 No online items Guide to the Stephen M. Cabrinety Collection in the History of Microcomputing, ca. 1975-1995 Processed by Stephan Potchatek; machine-readable finding aid created by Steven Mandeville-Gamble Department of Special Collections Green Library Stanford University Libraries Stanford, CA 94305-6004 Phone: (650) 725-1022 Email: [email protected] URL: http://library.stanford.edu/spc © 2001 The Board of Trustees of Stanford University. All rights reserved. Special Collections M0997 1 Guide to the Stephen M. Cabrinety Collection in the History of Microcomputing, ca. 1975-1995 Collection number: M0997 Department of Special Collections and University Archives Stanford University Libraries Stanford, California Contact Information Department of Special Collections Green Library Stanford University Libraries Stanford, CA 94305-6004 Phone: (650) 725-1022 Email: [email protected] URL: http://library.stanford.edu/spc Processed by: Stephan Potchatek Date Completed: 2000 Encoded by: Steven Mandeville-Gamble © 2001 The Board of Trustees of Stanford University. All rights reserved. Descriptive Summary Title: Stephen M. Cabrinety Collection in the History of Microcomputing, Date (inclusive): ca. 1975-1995 Collection number: Special Collections M0997 Creator: Cabrinety, Stephen M. Extent: 815.5 linear ft. Repository: Stanford University. Libraries. Dept. of Special Collections and University Archives. Language: English. Access Access restricted; this collection is stored off-site in commercial storage from which material is not routinely paged. Access to the collection will remain restricted until such time as the collection can be moved to Stanford-owned facilities. Any exemption from this rule requires the written permission of the Head of Special Collections.