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Other ORP type . 2021
License: CC BY
Data sources: Datacite
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Other ORP type . 2021
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Image fits files for Rapid-response radio observations of short GRB 181123B with the Australia Telescope Compact Array

Authors: Anderson, Gemma Elizabeth;

Image fits files for Rapid-response radio observations of short GRB 181123B with the Australia Telescope Compact Array

Abstract

Australia Telescope Compact Array (ATCA) fits Stokes I images of gamma-ray burst (GRB) 181123B. These fits images are from data obtained using the ATCA rapid-response system and began 12.6 hours following the Neil Gehrels Swift Observatory detection of GRB 181123B. The observations were taken at 5.5 and 9 GHz, integrating for 8.3 hours. No radio emission was detected in these data from this GRB. Two Stokes I fits images have been uploaded for each frequency. The files GRB181123B_5GHz_pbcorr.fits and GRB 181123B_9GHz_pbcorr.fits are the primary beam corrected images of the field of GRB 181123B at 5.5 and 9 GHz, respectively. The files GRB181123B_5GHz_sub_pbcorr.fits and GRB 181123B_9GHz_sub_pbcorr.fits are primary beam images of the same field but for which the clean model of all field sources was first subtracted from the visibilities.

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Keywords

radio continuum: transients, transients: gamma-ray bursts, transients: neutron star mergers, gamma-ray burst: individual: GRB 181123B

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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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