VizieR Online Data Catalog: Comparison between GRB afterglows and AT2017gfo (Rossi+, 2020)
Abstract
The follow-up with VLT/X-Shooter of AT2017gfo is not only the first spectroscopic observation of a KN, but it also provided the first temporal sampling of this new class of sources. The 10 spectra, described in Pian et al. (2017Natur.551...67P) and Smartt et al. (2017Natur.551...75S), were taken between ~1.5 and ~10.5d after the GW trigger and have a coverage from UV to NIR bands.
At epochs earlier than the first spectrum (i.e. <1.5d after the GW trigger), we have collected photometric observations from the works of Tanvir et al. (2017ApJ...848L..27T), Drout et al. (2017Sci...358.1570D), Evans et al. (2017Sci...358.1565E), Covino et al. (2017NatAs...1..791C), Coulter et al. (2017Sci...358.1556C), Troja et al. (2017Natur.551...71T), Pian et al. (2017Natur.551...67P), Cowperthwaite et al. (2017ApJ...848L..17C); see also the Kilonova Project: Guillochon et al. (2017ApJ...835...64G). Our starting sample of short GRBs is that presented by Fong et al. (2015ApJ...815..102F) which includes 87 short GRBs with optical and NIR counterparts observed between 2004 November and 2015 March. We considered only the 33 events that have a redshift determination. We extended this sample by including six short GRBs with known redshift, detected between 2015 March and 2019 June. (3 data files).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- April 2023
- Bibcode:
- 2023yCat..74933379R
- Keywords:
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- GRB;
- Gravitational wave;
- Photometry;
- Optical;
- Infrared