Analysis of {gamma}-ray bursts

DOI

To find out the astrophysical processes responsible for gamma-ray burst (GRB), it is crucial to discover and understand the relations between their observational properties. This work was performed in the GRB rest frames using a sample of 62 long Swift GRBs with known redshifts. Following the earlier analysis of the correlation between afterglow luminosity (L^^a) and break time (T^^a), we extend it to correlations between the afterglow and the prompt emission GRB physical parameters.

Cone search capability for table J/MNRAS/418/2202/table1 (*A data list for GRBs with known redshifts analysed in the paper)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74182202
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/418/2202
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/418/2202
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/418/2202
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/418/2202
Provenance
Creator Dainotti M.G.; Ostrowski M.; Willingale R.
Publisher CDS
Publication Year 2012
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Natural Sciences; Observational Astronomy; Physics