G
Gregory Y. Prigozhin
Researcher at Massachusetts Institute of Technology
Publications - 128
Citations - 6349
Gregory Y. Prigozhin is an academic researcher from Massachusetts Institute of Technology. The author has contributed to research in topics: Gamma-ray burst & Advanced CCD Imaging Spectrometer. The author has an hindex of 31, co-authored 117 publications receiving 5249 citations. Previous affiliations of Gregory Y. Prigozhin include Stanford University.
Papers
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Journal ArticleDOI
X-Ray Imaging Spectrometer (XIS) on Board Suzaku
Katsuji Koyama,Hiroshi Tsunemi,Tadayasu Dotani,Mark W. Bautz,Kiyoshi Hayashida,Takeshi Go Tsuru,Hironori Matsumoto,Yoshiaki Ogawara,George R. Ricker,John P. Doty,Steven E. Kissel,R. S. Foster,Hiroshi Nakajima,Hiroya Yamaguchi,Hideyuki Mori,Masaaki Sakano,Kenji Hamaguchi,Mamiko Nishiuchi,Emi Miyata,Ken'ichi Torii,M. Namiki,Satoru Katsuda,Daisuke Matsuura,Tomofumi Miyauchi,Naohisa Anabuki,Noriaki Tawa,Masanobu Ozaki,Hiroshi Murakami,Yoshitomo Maeda,Yoshinori Ichikawa,Gregory Y. Prigozhin,E. Boughan,Beverly LaMarr,Eric D. Miller,Barry E. Burke,J. A. Gregory,Allen D. Pillsbury,Aya Bamba,Junko S. Hiraga,Atsushi Senda,Haruyoshi Katayama,Shunji Kitamoto,Masahiro Tsujimoto,Takayoshi Kohmura,Yohko Tsuboi,Hisamitsu Awaki +45 more
TL;DR: The XIS is an X-ray imaging spectrometer system, consisting of state-of-the-art charge-coupled devices (CCDs) optimized for Xray detection, camera bodies, and control electronics as mentioned in this paper.
Journal ArticleDOI
PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
M. C. Miller,Frederick K. Lamb,Alexander J. Dittmann,Slavko Bogdanov,Zaven Arzoumanian,Keith C. Gendreau,Sebastien Guillot,Alice K. Harding,Wynn C. G. Ho,Wynn C. G. Ho,James M. Lattimer,Renee M. Ludlam,Simin Mahmoodifar,Simin Mahmoodifar,Sharon M. Morsink,Paul S. Ray,Tod E. Strohmayer,K. S. Wood,Teruaki Enoto,R. S. Foster,Takashi Okajima,Gregory Y. Prigozhin,Yang Soong +22 more
TL;DR: In this paper, the mass and radius of the isolated 205.53 Hz millisecond pulsar PSR J0030+0451 were estimated using a Bayesian inference approach to analyze its energy-dependent thermal X-ray waveform, which was observed using the Neutron Star Interior Composition Explorer (NICER).
Journal ArticleDOI
PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
M. C. Miller,Frederick K. Lamb,Alexander J. Dittmann,Slavko Bogdanov,Zaven Arzoumanian,Keith C. Gendreau,Sebastien Guillot,Alice K. Harding,Wynn C. G. Ho,Wynn C. G. Ho,James M. Lattimer,Renee M. Ludlam,Simin Mahmoodifar,Simin Mahmoodifar,Sharon M. Morsink,Paul S. Ray,Tod E. Strohmayer,K. S. Wood,Teruaki Enoto,R. S. Foster,Takashi Okajima,Gregory Y. Prigozhin,Yang Soong +22 more
TL;DR: In this article, the mass and radius of the isolated 205.53 Hz millisecond pulsar PSR J0030+0451 were estimated using a Bayesian inference approach to analyze its energy-dependent thermal X-ray waveform.
Proceedings ArticleDOI
The Neutron star Interior Composition Explorer (NICER): design and development
Keith C. Gendreau,Zaven Arzoumanian,Phillip Adkins,Cheryl L. Albert,John F. Anders,Andrew T. Aylward,Charles Baker,Erin Balsamo,William A. Bamford,Suyog S. Benegalrao,Daniel L. Berry,Shiraz Bhalwani,J. Kevin Black,Carl Blaurock,Ginger Bronke,Gary L. Brown,Jason Budinoff,Jeffrey D. Cantwell,Thoniel Cazeau,Philip T. Chen,Thomas G. Clement,Andrew T. Colangelo,Jerry S. Coleman,Jonathan D. Coopersmith,William E. Dehaven,John P. Doty,Mark Egan,Teruaki Enoto,Terry W.-M. Fan,Deneen M. Ferro,R. Foster,Nicholas M. Galassi,Luis D. Gallo,Christopher M. Green,Dave Grosh,Kong Q. Ha,Monther A. Hasouneh,Kristofer B. Heefner,Phyllis Hestnes,Lisa J. Hoge,Tawanda M. Jacobs,John Leif Jørgensen,Michael A. Kaiser,James W. Kellogg,Steven Kenyon,Richard Koenecke,Robert Kozon,Beverly LaMarr,Mike D. Lambertson,Anne M. Larson,Steven Lentine,Jesse Lewis,Michael G. Lilly,Kuochia Alice Liu,Andrew Malonis,Sridhar S. Manthripragada,Craig B. Markwardt,Bryan D. Matonak,Isaac E. Mcginnis,Roger L. Miller,Alissa L. Mitchell,Jason W. Mitchell,Jelila S. Mohammed,Charles Monroe,K Garcia,Peter Mule,Louis T. Nagao,Son N. Ngo,Eric D. Norris,Dwight A. Norwood,Joseph Novotka,Takashi Okajima,L. Olsen,Chimaobi O. Onyeachu,Henry Y. Orosco,Jacqualine R. Peterson,Kristina N. Pevear,Karen K. Pham,Sue E. Pollard,John S. Pope,Daniel Powers,Charles E. Powers,Samuel R. Price,Gregory Y. Prigozhin,Julian B. Ramirez,Winston J. Reid,Ronald A. Remillard,Eric M. Rogstad,Glenn P. Rosecrans,John N. Rowe,Jennifer A. Sager,Claude A. Sanders,Bruce Savadkin,Maxine R. Saylor,Alexander F. Schaeffer,Nancy S. Schweiss,Sean R. Semper,Peter J. Serlemitsos,Larry V. Shackelford,Yang Soong,Jonathan Struebel,Michael Vezie,Joel Villasenor,Luke Winternitz,George I. Wofford,Michael R. Wright,Mike Y. Yang,Wayne H. Yu +107 more
TL;DR: The Neutron star Interior Composition Explorer (NICER) mission is scheduled for launch in early 2017 on the Commercial Resupply Services SpaceX-11 flight.
Journal ArticleDOI
Discovery of the short |[gamma]|-ray burst GRB 050709
Joel Villasenor,D. Q. Lamb,George R. Ricker,J. L. Atteia,N. Kawai,N. Butler,Y. E. Nakagawa,J. G. Jernigan,M. Boer,Geoffrey B. Crew,T. Q. Donaghy,John P. Doty,E. E. Fenimore,M. Galassi,C. Graziani,Kevin Hurley,Al Levine,F. Martel,Masaru Matsuoka,J. F. Olive,Gregory Y. Prigozhin,T. Sakamoto,Y. Shirasaki,Motoko Suzuki,Toru Tamagawa,Roland Vanderspek,S. E. Woosley,A. Yoshida,João Braga,R. K. Manchanda,G. Pizzichini,K. Takagishi,Makoto Yamauchi +32 more
TL;DR: In this article, a short-hard gamma-ray burst (GRB 050509B) was detected by the Swift satellite, which measured its location and detected the X-ray afterglow, leading to the identification of the host galaxy of the burst as a late type galaxy at z = 0.16.