G
G. Chincarini
Researcher at INAF
Publications - 115
Citations - 8014
G. Chincarini is an academic researcher from INAF. The author has contributed to research in topics: Gamma-ray burst & Afterglow. The author has an hindex of 37, co-authored 115 publications receiving 7407 citations. Previous affiliations of G. Chincarini include University of Milano-Bicocca & University of Milan.
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Journal ArticleDOI
Methods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs
Phil Evans,A. P. Beardmore,K. L. Page,J. P. Osborne,P. T. O'Brien,Richard Willingale,R. L. C. Starling,David N. Burrows,Olivier Godet,L. Vetere,Judith Racusin,M. R. Goad,Klaas Wiersema,Lorella Angelini,Milvia Capalbi,G. Chincarini,G. Chincarini,Neil Gehrels,J. A. Kennea,Raffaella Margutti,Raffaella Margutti,D. C. Morris,D. C. Morris,C. J. Mountford,C. Pagani,M. Perri,P. Romano,Nial R. Tanvir +27 more
TL;DR: A homogeneous X-rays analysis of all 318 gamma-ray bursts detected by the X-ray telescope (XRT) on the Swift satellite up to 2008 July 23 is presented; this represents the largest sample ofX-ray GRB data published to date.
Journal ArticleDOI
Evidence for a Canonical Gamma-Ray Burst Afterglow Light Curve in the Swift XRT Data
J. A. Nousek,Chryssa Kouveliotou,Dirk Grupe,K. L. Page,Jonathan Granot,Enrico Ramirez-Ruiz,Sandeep K. Patel,Sandeep K. Patel,David N. Burrows,Vanessa Mangano,Scott Barthelmy,A. P. Beardmore,Sergio Campana,Milvia Capalbi,G. Chincarini,G. Chincarini,Giancarlo Cusumano,A. Falcone,Neil Gehrels,Paolo Giommi,M. R. Goad,Olivier Godet,Cheryl Hurkett,J. A. Kennea,Alberto Moretti,P. T. O'Brien,J. P. Osborne,P. Romano,Gianpiero Tagliaferri,Alan A. Wells +29 more
TL;DR: In this article, the early X-ray afterglows of the first 27 gamma-ray bursts (GRBs) well observed by the Swift X-Ray Telescope (XRT).
Journal ArticleDOI
The Early X-Ray Emission from GRBs
P. T. O'Brien,Richard Willingale,J. P. Osborne,M. R. Goad,K. L. Page,Simon Vaughan,Evert Rol,A. P. Beardmore,Olivier Godet,Cheryl Hurkett,Alan A. Wells,Bing Zhang,Shiho Kobayashi,David N. Burrows,John A. Nousek,J. A. Kennea,A. Falcone,Dirk Grupe,Neil Gehrels,Scott Barthelmy,J. K. Cannizzo,J. K. Cannizzo,Jay Cummings,Jay Cummings,J. E. Hill,J. E. Hill,Hans A. Krimm,Hans A. Krimm,G. Chincarini,G. Chincarini,Gianpiero Tagliaferri,Sergio Campana,Alberto Moretti,Paolo Giommi,M. Perri,Vanessa Mangano,V. LaParola +36 more
TL;DR: In this article, the early X-ray emission for a sample of 40 gamma-ray bursts (GRBs) obtained using the Swift satellite, for which the narrow-field instruments were pointed at the burst within 10 minutes of the trigger.
Journal ArticleDOI
SN 2003lw and GRB 031203: A Bright Supernova for a Faint Gamma-Ray Burst
D. Malesani,Gianpiero Tagliaferri,G. Chincarini,G. Chincarini,Stefano Covino,M. Della Valle,Dino Fugazza,Paolo A. Mazzali,Paolo A. Mazzali,Filippo Maria Zerbi,P. D'Avanzo,S. Kalogerakos,S. Kalogerakos,A. Simoncelli,A. Simoncelli,L. A. Antonelli,Luciano Burderi,Sergio Campana,A. Cucchiara,A. Cucchiara,Fabrizio Fiore,Giancarlo Ghirlanda,P. Goldoni,Diego Götz,Sandro Mereghetti,I. F. Mirabel,P. Romano,Luigi Stella,Takeo Minezaki,Yuzuru Yoshii,Ken'ichi Nomoto +30 more
TL;DR: In this paper, a very faint afterglow is detected superposed onto the host galaxy in the first infrared JHK observations, carried out ~9 hr after the burst, and a rebrightening is detected in all bands, peaking in the R band about 18 rest-frame days after burst.
Journal ArticleDOI
The Afterglows of Swift-era Gamma-ray Bursts. I. Comparing pre-Swift and Swift-era Long/Soft (Type II) GRB Optical Afterglows
David Alexander Kann,Sylvio Klose,Bing Zhang,D. B. Malesani,Ehud Nakar,Ehud Nakar,A. Pozanenko,A. C. Wilson,Nathaniel R. Butler,Pall Jakobsson,Pall Jakobsson,Steve Schulze,Maksim V. Andreev,L. A. Antonelli,I. F. Bikmaev,V. Biryukov,Markus Böttcher,R. A. Burenin,J. M. Castro Cerón,J. M. Castro Cerón,A. J. Castro-Tirado,G. Chincarini,G. Chincarini,B. E. Cobb,B. E. Cobb,Stefano Covino,P. D'Avanzo,Valerio D'Elia,M. Della Valle,M. Della Valle,A. de Ugarte Postigo,Yu. S. Efimov,P. Ferrero,Dino Fugazza,Johan P. U. Fynbo,M. Gålfalk,F. Grundahl,Javier Gorosabel,S. Gupta,Sergei Guziy,B. M. Hafizov,Jens Hjorth,K. Holhjem,Mansur Ibrahimov,Myungshin Im,G. L. Israel,M. Jeĺinek,B. L. Jensen,R. Karimov,Irek Khamitov,Ü. Kızıloǧlu,E. Klunko,Petr Kubánek,Alexander Kutyrev,Peter Laursen,Andrew J. Levan,Filippo Mannucci,C. M. Martin,A. Mescheryakov,Nestor Mirabal,Jay P. Norris,J. E. Ovaldsen,D. Paraficz,Elena P. Pavlenko,Silvia Piranomonte,Andrea Rossi,Vasilij Rumyantsev,R. Salinas,A. Sergeev,D. Sharapov,Jesper Sollerman,Jesper Sollerman,Bringfried Stecklum,Luigi Stella,Gianpiero Tagliaferri,Nial R. Tanvir,J. Telting,Vincenzo Testa,Adria C. Updike,A. Volnova,Darach Watson,Klaas Wiersema,Klaas Wiersema,Dong Xu +83 more
TL;DR: The first indications of a class of long GRBs are presented, which form a bridge between the typical high-luminosity, high-redshift events and nearby low- luminosity events (which are also associated with spectroscopic supernovae) in terms of energetics and observed redshift distribution, indicating a continuous distribution overall.