S
Shashi B. Pandey
Researcher at Aryabhatta Research Institute of Observational Sciences
Publications - 124
Citations - 3720
Shashi B. Pandey is an academic researcher from Aryabhatta Research Institute of Observational Sciences. The author has contributed to research in topics: Gamma-ray burst & Light curve. The author has an hindex of 31, co-authored 114 publications receiving 3320 citations. Previous affiliations of Shashi B. Pandey include University of Michigan & Central Drug Research Institute.
Papers
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Journal ArticleDOI
Photometric calibration of the Swift ultraviolet/optical telescope
T. S. Poole,A. A. Breeveld,M. J. Page,Wayne B. Landsman,Stephen T. Holland,Stephen T. Holland,P. W. A. Roming,N. P. M. Kuin,Peter J. Brown,Caryl Gronwall,S. D. Hunsberger,S. Koch,Keith O. Mason,Keith O. Mason,Patricia Schady,D. E. Vanden Berk,A. J. Blustin,P. Boyd,Patrick S. Broos,M. Carter,M. M. Chester,Antonino Cucchiara,B. Hancock,H. Huckle,Stefan Immler,M. Ivanushkina,T. Kennedy,Frank Marshall,Adam N. Morgan,Shashi B. Pandey,M. de Pasquale,Philip J. Smith,M. Still +32 more
TL;DR: In this article, the photometric calibration of the Swift Ultraviolet/Optical Telescope (UVOT) was performed with observations of standard stars and standard star fields that represent a wide range of spectral star types.
Journal ArticleDOI
Thirty Meter Telescope Detailed Science Case: 2015
Warren Skidmore,Ian P. Dell'Antonio,Misato Fukugawa,Aruna Goswami,Lei Hao,David Jewitt,Greg Laughlin,Charles C. Steidel,Paul Hickson,Luc Simard,M. Schöck,Tommaso Treu,Judith G. Cohen,G. C. Anupama,Mark Dickinson,Fiona A. Harrison,Tadayuki Kodama,Jessica R. Lu,Bruce Macintosh,Matthew A. Malkan,Shude Mao,Norio Narita,Tomohiko Sekiguchi,Annapurni Subramaniam,Masaomi Tanaka,Feng Tian,Michael F. A'Hearn,Masayuki Akiyama,Babar Ali,Wako Aoki,Manjari Bagchi,Aaron J. Barth,Varun Bhalerao,Marusa Bradac,James S. Bullock,Adam J. Burgasser,Scott Chapman,Ranga-Ram Chary,Masashi Chiba,Michael C. Cooper,Asantha Cooray,Ian J. M. Crossfield,Thayne Currie,Mousumi Das,Gulab C. Dewangan,Richard de Grijs,Tuan Do,Subo Dong,Jarah Evslin,Taotao Fang,Xuan Fang,Christopher D. Fassnacht,Leigh N. Fletcher,Eric Gaidos,Roy R. Gal,Andrea M. Ghez,Mauro Giavalisco,Carol A. Grady,Thomas K. Greathouse,Rupjyoti Gogoi,Puragra Guhathakurta,Luis C. Ho,Priya Hasan,Gregory J. Herczeg,Mitsuhiko Honda,Masa Imanishi,Hanae Inami,Masanori Iye,Jason S. Kalirai,U.S. Kamath,Stephen R. Kane,Nobunari Kashikawa,Mansi M. Kasliwal,Vishal P. Kasliwal,Evan N. Kirby,Quinn Konopacky,Sébastien Lépine,Di Li,Jianyang Li,Junjun Liu,Michael C. Liu,Enrigue Lopez-Rodriguez,Jennifer M. Lotz,Philip Lubin,Lucas M. Macri,Keiichi Maeda,Franck Marchis,Christian Marois,Alan P. Marscher,Crystal L. Martin,Taro Matsuo,Claire E. Max,Alan W. McConnachie,Stacy McGough,Carl Melis,Leo Meyer,Michael J. Mumma,Takayuki Muto,Tohru Nagao,Joan Najita,Julio F. Navarro,Michael J. Pierce,Jason X. Prochaska,Masamune Oguri,Devendra K. Ojha,Yoshiko K. Okamoto,Glenn S. Orton,Angel Otarola,Masami Ouchi,Chris Packham,Deborah Padgett,Shashi B. Pandey,Catherine Pilachowsky,Klaus M. Pontoppidan,Joel R. Primack,Shalima Puthiyaveettil,Enrico Ramirez-Ruiz,Naveen A. Reddy,Michael Rich,Matthew J. Richter,James Schombert,Anjan A. Sen,Jianrong Shi,Kartik Sheth,Raghunathan Srianand,Jonathan C. Tan,Masayuki Tanaka,Angelle Tanner,Nozomu Tominaga,David Tytler,Vivian U,Lingzhi Wang,Xiaofeng Wang,Yiping Wang,Gillian Wilson,Shelley A. Wright,Chao Wu,Xufeng Wu,Renxin Xu,Toru Yamada,Bin Yang,Gongbo Zhao,Hongsheng Zhao +142 more
TL;DR: The TMT Detailed Science Case describes the transformational science that the Thirty Meter Telescope (TMT) will enable as mentioned in this paper, and more than 150 astronomers from within the TMT partnership and beyond offered input in compiling the new 2015 detailed science case, including the California Institute of Technology (Caltech), the Indian Institute of Astrophysics (IIA), the National Astronomical Observatories of the Chinese Academy of Sciences (NAOC), the NaOJ, the University of California, the Association of Canadian Universities for Research in Astronomy (ACURA) and US associate partner, AU
Journal ArticleDOI
Transition from fireball to Poynting-flux-dominated outflow in the three-episode GRB 160625B
Ignacio de Gregorio Monsalvo,Ignacio de Gregorio Monsalvo,Bin-Bin Zhang,Bin-Bin Zhang,Aleksander Filip Żarnecki,Bing Zhang,Bing Zhang,A. J. Castro-Tirado,A. J. Castro-Tirado,Zi-Gao Dai,P.-H. T. Tam,X.-Y. Wang,Y. D. Hu,Y. D. Hu,Sergey Karpov,Sergey Karpov,Alexei Pozanenko,Alexei Pozanenko,Alexei Pozanenko,Fu-Wen Zhang,E. Mazaeva,P. Minaev,A. Volnova,S. R. Oates,S. R. Oats,S. R. Oats,He Gao,Xue-Feng Wu,Xue-Feng Wu,Xue-Feng Wu,Lijing Shao,Lijing Shao,Qing-Wen Tang,Gregory Beskin,Gregory Beskin,Anton Biryukov,Anton Biryukov,Sergey Bondar,E. Ivanov,E. Katkova,N. Orekhova,A. Perkov,Sasyuk,Lech Mankiewicz,Aleksander Filip Zarnecki,A. Cwiek,R. Opiela,A. K. Zadrożny,R. Aptekar,D. D. Frederiks,Dmitry S. Svinkin,A. Kusakin,R. Inasaridze,O. Burhonov,Rumyantsev,E. Klunko,A. S. Moskvitin,T. A. Fatkhullin,Sokolov,A. F. Valeev,A. F. Valeev,S. Jeong,S. Jeong,Il Han Park,M. D. Caballero-Garcia,Ronan Cunniffe,J. C. Tello,P. Ferrero,Shashi B. Pandey,Martin Jelínek,R. Sanchez-Ramirez,A. Castellon +71 more
TL;DR: In this paper, an extremely bright gamma-ray burst (GRB) 160625B was observed in both gamma and optical wavelengths, with three isolated episodes separated by long quiescent intervals, with the durations of each sub-burst being approximately 0.8, 35, and 212 seconds.
Journal ArticleDOI
Swift observations of GRB 060614: an anomalous burst with a well behaved afterglow
Vanessa Mangano,Stephen T. Holland,Stephen T. Holland,D. B. Malesani,Eleonora Troja,Eleonora Troja,Eleonora Troja,G. Chincarini,G. Chincarini,Bing Zhang,V. La Parola,V. La Parola,Peter J. Brown,David N. Burrows,Sergio Campana,Milvia Capalbi,Gaspare Cusumano,M. Della Valle,Neil Gehrels,Paolo Giommi,Dirk Grupe,C. Guidorzi,C. Guidorzi,Teresa Mineo,Alberto Moretti,J. P. Osborne,Shashi B. Pandey,M. Perri,P. Romano,P. Romano,P. W. A. Roming,Gianpiero Tagliaferri +31 more
TL;DR: Spectral analysis of the Swift observations of GRB 060614 shows that the burst presents standard optical, ultraviolet and X-ray afterglows, detected beginning 4 ks after the trigger, and that the peak energy of the burst has decreased to as low as 8 keV at the beginning of the XRT observation.
Journal ArticleDOI
Optical and near-infrared observations of the GRB020405 afterglow ?
N. Masetti,Eliana Palazzi,Elena Pian,A. Simoncelli,Leslie K. Hunt,E. Maiorano,Andrew J. Levan,Lise Christensen,Evert Rol,Sandra Savaglio,Sandra Savaglio,Renato Falomo,A. J. Castro-Tirado,Jens Hjorth,A. Delsanti,Maurilio Pannella,Vijay Mohan,Shashi B. Pandey,Ram Sagar,Lorenzo Amati,I. Burud,J. M. Castro Cerón,Filippo Frontera,A. S. Fruchter,Johan P. U. Fynbo,Javier Gorosabel,Lex Kaper,Sylvio Klose,Chryssa Kouveliotou,Luciano Nicastro,Holger Pedersen,James E. Rhoads,I. Salamanca,Nial R. Tanvir,Paul Vreeswijk,Ralph A. M. J. Wijers,E.P.J. van den Heuvel +36 more
TL;DR: It is suggested that the bump can be modeled with a SN having the same temporal profile as the other proposed hypernova SN2002ap, but 1.3 mag brighter at peak, and located at the GRB redshift.