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The Afterglow and Environment of the Short Grb 111117a
... of short GRB 111117A at δt ≈ 3 d, which leads to a robust association with a galaxy at a photometric redshift of z ≈ ...Among short GRBs, only GRBs 050724 and 051221A were detected at later ... See full document
12
Broadband Observations of the Afterglow of GRB : Observing the Effect of Inverse Compton Scattering
... Broadband afterglow observa- tions, spanning from X-ray to radio frequencies, provide a probe of the density structure of the circumburst medium, as well as of the ejecta energetics, geometry, and the physical ... See full document
17
GRB 050408: A bright gamma-ray burst probing an atypical galactic environment
... other afterglow spectra (Savaglio & Fall 2004; Vreeswijk et ...the GRB may have resulted in the destruction of the dust ...the GRB event (Waxman & Draine ... See full document
14
The optical afterglow of the short gamma-ray burst associated with GW170817
... research environment grant “Gravitational Radiation and Electromagnetic Astrophysical Tran- sients (GREAT)” funded by the Swedish Research council (VR) under Dnr ... See full document
23
An unusual transient following the short GRB 071227
... while GRB 071227 appears to decay as a simple power ...than, GRB 060614 cannot be totally discounted. In the r band, GRB 060614 is almost an order of magnitude brighter than that observed in the ... See full document
16
Gemini spectroscopy of the short-hard gamma-ray burst GRB 130603b afterglow and host galaxy
... the afterglow exhibits weak Ca ii absorption features but negligible emission ...of short-duration GRB hosts and with recent results which suggest GRB 130603B emission to be the product of the ... See full document
8
The optical afterglow and host galaxy of GRB ,,
... X-ray afterglow (Costa et ...in GRB research. The determination of a redshift of 0.835 for GRB 970508 (Metzger et ...the environment of GRBs and to possibly shed some light on the nature of ... See full document
9
Happy Birthday Swift: Ultra-Long GRB 141121A and its Broadband Afterglow
... of GRB 141121A, which was discovered by the Swift satellite and observed starting a few hours after the explosion and continuing over the following ...model. GRB 141121A is expanding in a wind-like ... See full document
13
A REVERSE SHOCK in GRB 160509A
... -LAT GRB 160509A at z = ...the afterglow emission comprises distinct reverse shock and forward shock contributions: the reverse shock emission dominates in the radio band at ...circumburst ... See full document
8
GRB 130427A Afterglow: A Test for GRB Models
... the afterglow of the exceptionally luminous GRB 130427A, which took place up to 90 Ms from the ...X-ray afterglow of a cosmological ...density environment (K13) as well, or evolving and ... See full document
12
The luminous infrared host galaxy of short-duration GRB 100206A
... low short-GRB event rate (<10 events yr −1 ) and uncertain selection biases affecting the population (∼25% of all Swift short GRBs are not detected by the X-Ray Telescope (XRT) and cannot be ... See full document
15
Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z = 3.2 gamma-ray burst
... Most of the lines were fitted from the combined 600V spec- trum which covers all metal absorption lines detected longwards of Ly-α, but provides a higher resolution than the 300V spectra. The 600I spectra only covers the ... See full document
21
The 80 Ms follow up of the X ray afterglow of GRB 130427A challenges the standard forward shock model
... the GRB trigger. The high energetics and low redshift of GRB 130427A have enabled X-ray observations to be obtained over a much longer and unprecedented time-scale after the initial trigger, which allows us ... See full document
13
The Unusually Long Duration Gamma-ray Burst GRB 000911: Discovery of the afterglow and host galaxy
... and Analysis Facility (IRAF). 13 Aperture photometry was used to measure the magnitude of the optical afterglow in each image. Photometric zero points for the Keck imaging were based on stars in the field, with ... See full document
7
The 2175 angstrom Extinction Feature in the Optical Afterglow Spectrum of GRB 180325A at z =. 2.25
... (GRB) afterglow GRB 180325A at ...of GRB follow-up, at four different epochs with the Nordic Optical Telescope (NOT) and the Very Large Telescope ...the afterglow are obtained with the ... See full document
9
Reactions of short lived species in a flowing afterglow
... To measure the rate constants for reactions in which both the ionic and neutral species have thermal distributions of kinetic energy, the pulsed ion source has been developed.3 1 Ions ar[r] ... See full document
174
The Supercritical Pile Gamma-Ray Burst Model: The GRB Afterglow Steep Decline and Plateau Phase
... the GRB “central engine”; such collisions are thought to be necessary in order to produce the observed rapid GRB variability (see, however, Narayan & Kumar 2009 ) and spectra with characteristic ... See full document
8
Revealing Short GRB Jet Structure and Dynamics with Gravitational Wave Electromagnetic Counterparts
... the GRB will be sup- pressed resulting in a failed-GRB and an afterglow-like ...a GRB afterglow but without the prompt high-energy trigger ... See full document
9
Early time optical polarization of GRB Afterglows: GRB 060418 and GRB 090102
... of GRB 060418 (where a 2σ upper limit of P < 8 % was determined) and GRB 090102 (when a detection of P 10 ± 1 % was ...of GRB jet magnetization and describe a possible unified model that can ... See full document
6
The Onset of Gamma-Ray Burst Afterglow
... a short burst GRB 050724 (Barthelmy et ...multiple short BATSTE GRBs, and it might be the onset of short burst afterglow (Lazzati, Ramirez-Ruiz & Ghisellini ... See full document
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