Difference: GCNCIRCULAR21588 ( vs. 1)

Revision 12017-08-19 - ShaonGhosh

Line: 1 to 1
Added:
>
>
META TOPICPARENT name="LVCGCNs"
TITLE: GCN CIRCULAR
NUMBER: 21588
SUBJECT: LIGO/Virgo G298048: VLBA observations of the possible counterpart SSS17a in NGC 4993
DATE: 17/08/19 09:36:26 GMT
FROM: Igor Andreoni at Swinburne U of Tech <igor.andreoni@gmail.com>

A. Deller (Swinburne/OzGrav), M. Bailes (Swinburne/OzGrav), I. Andreoni (Swinburne/OzGrav/AAO), K. Bannister (CSIRO), J. Cooke (Swinburne/OzGrav), D. Dobie (University of Sydney), D. Kaplan (UWM) C. Lynch (University of Sydney), T. Murphy (University of Sydney), on behalf of a joint effort between OzGrav and the VAST collaboration.

We are observing the optical transient SSS17a (Coulter et al. - GCN 21529, Allam et al. - GCN 21530, Yang et al.- GCN 21531, Melandri et al. - GCN 21532) and its host galaxy NGC 4993 with the Very Long Baseline Array.

We are observing at a central frequency of 8.7 GHz with a bandwidth of 256 MHz.

The first observation took place from 2017-08-17 19:58UT to 2017-08-18 01:34UT.

Analysis of the data will take place after correlation, in 7-10 days.

Two subsequent epochs are planned in the coming three days.

We thank the Long Baseline Observatory staff for facilitating these observations.

-- ShaonGhosh - 19 Aug 2017

 
This site is powered by the TWiki collaboration platform Powered by PerlCopyright © 2008-2025 by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
Ideas, requests, problems regarding TWiki? Send feedback