GCN Circular 24215
Subject
LIGO/Virgo S190425z - ePESSTO+ NTT spectrum of candidate PS19qo
Date
2019-04-26T07:11:30Z (5 years ago)
From
Matt Nicholl at Royal Astronomical Soc. <mrn@roe.ac.uk>
P. Short, M. Nicholl (Edinburgh), S. J. Smartt, K. W. Smith (QUB), K. Chambers, M. Huber (IfA) , J. Anderson (ESO), T.-W. Chen (MPE), C. Inserra (Cardiff), O. Yaron (Weizmann), D. R. Young (QUB), C. Angus, M. Pursiainen, P. Wiseman (Southampton), S. Taubenberger (MPA), M. Gromadzki (Warsaw) on behalf of the ePESSTO+ collaboration
We observed PS19qo (Smith et al., GCN 24210) a potential counterpart to the gravitational wave trigger S190425z (GCN 24168), under the advanced Public ESO Spectroscopic Survey for Transient Objects (ePESSTO+; see Smartt et al. 2015, A&A, 579, 40 http://www.pessto.org). The observations were performed on the ESO New Technology Telescope at La Silla with the EFOSC2 instrument.
This candidate was chosen because of its apparent association with a cataloged galaxy at 199 Mpc. The NTT spectrum gives a good match to normal Type II SN at z=0.057.