Views provided by UsageCounts
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.
radio continuum: transients, transients: gamma-ray bursts, transients: neutron star mergers, gamma-ray burst: individual: GRB 181123B
radio continuum: transients, transients: gamma-ray bursts, transients: neutron star mergers, gamma-ray burst: individual: GRB 181123B
| selected citations These citations are derived from selected sources. 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). | 1 | |
| 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. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
| views | 5 |

Views provided by UsageCounts