M
M. de Pasquale
Researcher at Istanbul University
Publications - 189
Citations - 10328
M. de Pasquale is an academic researcher from Istanbul University. The author has contributed to research in topics: Gamma-ray burst & Afterglow. The author has an hindex of 50, co-authored 180 publications receiving 9422 citations. Previous affiliations of M. de Pasquale include University College London & University of Nevada, Las Vegas.
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
A short γ-ray burst apparently associated with an elliptical galaxy at redshift z = 0.225
Neil Gehrels,Craig L. Sarazin,P. T. O'Brien,Bing Zhang,L. M. Barbier,Scott Barthelmy,A. J. Blustin,David N. Burrows,J. K. Cannizzo,J. K. Cannizzo,Jay Cummings,Jay Cummings,Michael R. Goad,Stephen T. Holland,Stephen T. Holland,Cheryl Hurkett,J. A. Kennea,Andrew J. Levan,C. B. Markwardt,C. B. Markwardt,Keith O. Mason,Peter Mészáros,M. J. Page,David Palmer,Evert Rol,T. Sakamoto,T. Sakamoto,Richard Willingale,Lorella Angelini,Lorella Angelini,Andrew P. Beardmore,Patricia T. Boyd,Patricia T. Boyd,A. A. Breeveld,Sergio Campana,M. M. Chester,Guido Chincarini,Guido Chincarini,L. R. Cominsky,Giancarlo Cusumano,M. de Pasquale,Edward E. Fenimore,Paolo Giommi,Caryl Gronwall,Dirk Grupe,Joanne E. Hill,D. Hinshaw,Jens Hjorth,D. Hullinger,D. Hullinger,Kevin Hurley,Sylvio Klose,Shiho Kobayashi,Chryssa Kouveliotou,Hans A. Krimm,Hans A. Krimm,Vanessa Mangano,F. E. Marshall,Katherine E. McGowan,A. Moretti,Richard Mushotzky,Kazuhiro Nakazawa,Jay P. Norris,John A. Nousek,J. P. Osborne,K. L. Page,A. M. Parsons,Sandeep K. Patel,M. Perri,T. S. Poole,P. Romano,P. W. A. Roming,Stuart Rosen,G. Sato,Patricia Schady,Alan P. Smale,Jesper Sollerman,R. L. C. Starling,Martin Still,Martin Still,Masaya Suzuki,Gianpiero Tagliaferri,Tadayuki Takahashi,Makoto Tashiro,Jack Tueller,Alan A. Wells,Nicholas E. White,Ralph A. M. J. Wijers +87 more
TL;DR: In this article, the authors reported the detection of the X-ray afterglow from the short burst GRB 050509B and its location on the sky is near a luminous, non-star-forming elliptical galaxy at a redshift of 0.225.
Journal ArticleDOI
GRB 090423 at a redshift of z ≈ 8.1
Ruben Salvaterra,M. Della Valle,Sergio Campana,G. Chincarini,G. Chincarini,Stefano Covino,P. D'Avanzo,P. D'Avanzo,Alberto Fernández-Soto,C. Guidorzi,Filippo Mannucci,Raffaella Margutti,Raffaella Margutti,Christina C. Thöne,L. A. Antonelli,Scott Barthelmy,M. de Pasquale,V. D'Elia,Fabrizio Fiore,Dino Fugazza,L. K. Hunt,Elisabetta Maiorano,S. Marinoni,F. E. Marshall,Emilio Molinari,J. A. Nousek,Elena Pian,Judith Racusin,Luigi Stella,Lorenzo Amati,Gloria Andreuzzi,Giancarlo Cusumano,E. E. Fenimore,P. Ferrero,P. Giommi,Dafne Guetta,Stephen T. Holland,Stephen T. Holland,Kevin Hurley,G. L. Israel,J. Mao,C. B. Markwardt,C. B. Markwardt,N. Masetti,C. Pagani,Eliana Palazzi,D. M. Palmer,Silvia Piranomonte,Gianpiero Tagliaferri,Vincenzo Testa +49 more
TL;DR: Tanvir et al. as mentioned in this paper used the United Kingdom Infrared Telescope, Hawaii, from about 20 minutes after the burst and arrive at z ≈ 8.2, implying that massive stars were being produced and dying as GRBs approximately 620 million years after the Big Bang.
Journal ArticleDOI
An extremely luminous X-ray outburst at the birth of a supernova
Alicia M. Soderberg,Alicia M. Soderberg,Edo Berger,Edo Berger,K. L. Page,Patricia Schady,Jerod T. Parrent,David Pooley,Xiang-Yu Wang,Eran O. Ofek,A. Cucchiara,A. Rau,Eli Waxman,Joshua D. Simon,Douglas C.-J. Bock,Peter Milne,M. J. Page,J. C. Barentine,Scott Barthelmy,A. P. Beardmore,Michael Bietenholz,Peter J. Brown,Adam Burrows,David N. Burrows,G. Byrngelson,Stephen Bradley Cenko,Poonam Chandra,Jay Cummings,D. B. Fox,Avishay Gal-Yam,Neil Gehrels,Stefan Immler,Mansi M. Kasliwal,Albert K. H. Kong,Hans A. Krimm,Hans A. Krimm,Shrinivas R. Kulkarni,Thomas J. Maccarone,Peter Mészáros,Ehud Nakar,P. T. O'Brien,Roderik Overzier,M. de Pasquale,Judith Racusin,Nanda Rea,Donald G. York +45 more
TL;DR: This work reports the serendipitous discovery of a supernova at the time of the explosion, marked by an extremely luminous X-ray outburst, and attributes the outburst to the ‘break-out’ of the supernova shock wave from the progenitor star, and shows that the inferred rate of such events agrees with that of all core-collapse supernovae.
Journal ArticleDOI
Swift and NuSTAR observations of GW170817: Detection of a blue kilonova.
Phil Evans,S. B. Cenko,S. B. Cenko,J. A. Kennea,S. W. K. Emery,N. P. M. Kuin,Oleg Korobkin,Ryan Wollaeger,Chris L. Fryer,K. K. Madsen,Fiona A. Harrison,Y. Xu,Ehud Nakar,Kenta Hotokezaka,A. Y. Lien,A. Y. Lien,Sergio Campana,S. R. Oates,Eleonora Troja,Eleonora Troja,A. A. Breeveld,Frank Marshall,Scott Barthelmy,A. P. Beardmore,David N. Burrows,Giancarlo Cusumano,Antonino D'Ai,P. D'Avanzo,Valerio D'Elia,Valerio D'Elia,M. de Pasquale,Wesley Even,Wesley Even,Christopher J. Fontes,Karl Forster,Javier A. García,Paolo Giommi,Brian W. Grefenstette,Caryl Gronwall,Dieter H. Hartmann,Marianne Heida,Aimee Hungerford,Mansi M. Kasliwal,Hans A. Krimm,Hans A. Krimm,Andrew J. Levan,D. B. Malesani,A. Melandri,Hiromasa Miyasaka,J. A. Nousek,P. T. O'Brien,J. P. Osborne,C. Pagani,K. L. Page,David Palmer,M. Perri,M. Perri,Sean N. Pike,Judith Racusin,Stephan Rosswog,Michael H. Siegel,T. Sakamoto,B. Sbarufatti,Gianpiero Tagliaferri,Nial R. Tanvir,A. Tohuvavohu +65 more
TL;DR: In this paper, ultraviolet and x-ray observations from the Nuclear Spectroscopic Telescope Array (NSTA) of the binary neutron star merger GW170817 were used to detect a high mass (≈0.03 solar masses) wind-driven outflow with moderate electron fraction.