scholarly journals The Observed Offset Distribution of Gamma-Ray Bursts from Their Host Galaxies: A Robust Clue to the Nature of the Progenitors

2002 ◽  
Vol 123 (3) ◽  
pp. 1111-1148 ◽  
Author(s):  
J. S. Bloom ◽  
S. R. Kulkarni ◽  
S. G. Djorgovski
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Host Galaxies

scholarly journals The Redshift Dependence of the Radio Flux of Gamma-Ray Bursts and Their Host Galaxies

2018 ◽  
Vol 865 (2) ◽  
pp. 82 ◽  
Author(s):  
Z. B. Zhang ◽  
P. Chandra ◽  
Y. F. Huang ◽  
D. Li
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Radio Flux ◽  
Host Galaxies

scholarly journals Constraints on the circumburst environments of short gamma-ray bursts

2020 ◽  
Vol 495 (4) ◽  
pp. 4782-4799 ◽  
Author(s):  
Brendan O’Connor ◽  
Paz Beniamini ◽  
Chryssa Kouveliotou
Keyword(s):  
Gamma Ray ◽  
Galactic Halo ◽  
Gamma Ray Bursts ◽  
Light Curves ◽  
Host Galaxy ◽  
Host Galaxies ◽  
Binary Neutron Star ◽  
Range Of Values ◽  
Short Grbs

ABSTRACT Observational follow up of well localized short gamma-ray bursts (SGRBs) has left $20\!-\!30{{\ \rm per\ cent}}$ of the population without a coincident host galaxy association to deep optical and NIR limits (≳26 mag). These SGRBs have been classified as observationally hostless due to their lack of strong host associations. It has been argued that these hostless SGRBs could be an indication of the large distances traversed by the binary neutron star system (due to natal kicks) between its formation and its merger (leading to an SGRB). The distances of GRBs from their host galaxies can be indirectly probed by the surrounding circumburst densities. We show that a lower limit on those densities can be obtained from early afterglow light curves. We find that ${\lesssim}16{{\ \rm per\ cent}}$ of short GRBs in our sample took place at densities ≲10−4 cm−3. These densities represent the expected range of values at distances greater than the host galaxy’s virial radii. We find that out of the five SGRBs in our sample that have been found to be observationally hostless, none are consistent with having occurred beyond the virial radius of their birth galaxies. This implies one of two scenarios. Either these observationally hostless SGRBs occurred outside of the half-light radius of their host galaxy, but well within the galactic halo, or in host galaxies at moderate to high redshifts (z ≳ 2) that were missed by follow-up observations.

scholarly journals A deep search for the host galaxies of gamma-ray bursts with no detected optical afterglow

2012 ◽  
Vol 545 ◽  
pp. A77 ◽  
Author(s):  
A. Rossi ◽  
S. Klose ◽  
P. Ferrero ◽  
J. Greiner ◽  
L. A. Arnold ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Host Galaxies

scholarly journals The cosmic gamma-ray bursts and their host galaxies in a cosmological context

2003 ◽  
Author(s):  
Stan G. Djorgovski ◽  
Shrinivas R. Kulkarni ◽  
Dale A. Frail ◽  
Fiona A. Harrison ◽  
Joshua S. Bloom ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Host Galaxies ◽  
Cosmological Context

scholarly journals Radio afterglows and host galaxies of gamma-ray bursts

2015 ◽  
Vol 451 (2) ◽  
pp. 1815-1823 ◽  
Author(s):  
Long-Biao Li ◽  
Zhi-Bin Zhang ◽  
Yong-Feng Huang ◽  
Xue-Feng Wu ◽  
Si-Wei Kong ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Host Galaxies

scholarly journals DESAlert: Enabling Real-Time Transient Follow-Up with Dark Energy Survey Data

2016 ◽  
Vol 33 ◽  
Author(s):  
A. Poci ◽  
K. Kuehn ◽  
T. Abbott ◽  
F. B. Abdalla ◽  
S. Allam ◽  
...  
Keyword(s):  
Dark Energy ◽  
Real Time ◽  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Host Galaxies ◽  
Gamma Ray Burst ◽  
Dark Energy Survey ◽  
Data Products ◽  
Energy Survey

AbstractThe Dark Energy Survey is undertaking an observational programme imaging 1/4 of the southern hemisphere sky with unprecedented photometric accuracy. In the process of observing millions of faint stars and galaxies to constrain the parameters of the dark energy equation of state, the Dark Energy Survey will obtain pre-discovery images of the regions surrounding an estimated 100 gamma-ray bursts over 5 yr. Once gamma-ray bursts are detected by, e.g., the Swift satellite, the DES data will be extremely useful for follow-up observations by the transient astronomy community. We describe a recently-commissioned suite of software that listens continuously for automated notices of gamma-ray burst activity, collates information from archival DES data, and disseminates relevant data products back to the community in near-real-time. Of particular importance are the opportunities that non-public DES data provide for relative photometry of the optical counterparts of gamma-ray bursts, as well as for identifying key characteristics (e.g., photometric redshifts) of potential gamma-ray burst host galaxies. We provide the functional details of the DESAlert software, and its data products, and we show sample results from the application of DESAlert to numerous previously detected gamma-ray bursts, including the possible identification of several heretofore unknown gamma-ray burst hosts.

scholarly journals Host galaxies of gamma-ray bursts: Spectral energy distributions and internal extinction

2001 ◽  
Vol 372 (2) ◽  
pp. 438-455 ◽  
Author(s):  
V. V. Sokolov ◽  
T. A. Fatkhullin ◽  
A. J. Castro-Tirado ◽  
A. S. Fruchter ◽  
V. N. Komarova ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Spectral Energy ◽  
Host Galaxies ◽  
Spectral Energy Distributions ◽  
Energy Distributions

scholarly journals Metallicity properties of the simulated host galaxies of long gamma-ray bursts and the fundamental metallicity relation

2011 ◽  
Vol 417 (2) ◽  
pp. 1013-1021 ◽  
Author(s):  
M. A. Campisi ◽  
C. Tapparello ◽  
R. Salvaterra ◽  
F. Mannucci ◽  
M. Colpi
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Host Galaxies

scholarly journals Host galaxies of long gamma-ray bursts in the Millennium Simulation

2010 ◽  
Vol 408 (1) ◽  
pp. 647-656 ◽  
Author(s):  
N. E. Chisari ◽  
P. B. Tissera ◽  
L. J. Pellizza
Keyword(s):  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Host Galaxies
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