REVIEW 1 cited by
The GRBSN webtool: An open-source repository for gamma-ray burst-supernova associations
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
The GRBSN webtool: An open-source repository for gamma-ray burst-supernova associations
read the original abstract
This paper presents the GRBSN webtool, an open-source data repository coupled to a web interface that hosts the most complete dataset of GRB-SN associations to date. In contrast to repositories of supernova (SN) or gamma-ray burst (GRB) data, this tool provides a multi-wavelength view of each GRB-SN association. GRBSN allows users to view and interact with plots of the data; search and filter the whole database; and download radio, X-ray, optical/NIR photometric and spectroscopic data related to a GRB-SN association. The web interface code and GRB-SN data are hosted on a public GitHub repository, allowing users to upload their own data, flag missing data and suggest improvements. The GRBSN webtool will be maintained by the Space Science group at University College Dublin, Ireland. As the number of confirmed GRB-SN associations increases in the coming years, the GRBSN webtool will provide a robust framework in which to catalogue these associations and their associated data. The web interface is available at: https://grbsn.watchertelescope.ie.
Forward citations
Cited by 1 Pith paper
-
AT2019ijn: a fast-rising, slow-decaying blue optical transient with exceptionally bright radio emission
AT2019ijn combines LFBOT-like fast optical rise and blue color with slow decay and radio luminosity peaking late at 2e31 erg/s/Hz, best fit as an off-axis jetted IMBH TDE.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.