GCN Circular 24198
Subject
LIGO/Virgo S190425z: KPED Follow-Up Observations
Date
2019-04-25T21:54:41Z (6 years ago)
From
Tomas Ahumada at U. of Maryland <tahumada@astro.umd.edu>
Authors: Tomas Ahumada (UMD), Michael W. Coughlin (Caltech), Kai Staats
(Embry-Riddle University), Richard G. Dekany
<https://arxiv.org/search/astro-ph?searchtype=author&query=Dekany%2C+R+G>
(Caltech), Dmitry A. Duev
<https://arxiv.org/search/astro-ph?searchtype=author&query=Duev%2C+D+A>
(Caltech), Michael Feeney
<https://arxiv.org/search/astro-ph?searchtype=author&query=Feeney%2C+M>
(Caltech), S. R. Kulkarni
<https://arxiv.org/search/astro-ph?searchtype=author&query=Kulkarni%2C+S+R>
(Caltech), Reed Riddle
<https://arxiv.org/search/astro-ph?searchtype=author&query=Riddle%2C+R>
(Caltech) on behalf of the KPED team and the Global Relay of Observatories
Watching Transients Happen (GROWTH) collaboration.
We used the Kitt Peak EMCCD Demonstrator (KPED) on the Kitt Peak 84-inch
telescope (Coughlin et al 2019b) to obtain 300 s r-band images for 10
galaxies in the 90% localization region of the S190425z LIGO/Virgo
detection (GCN 24168). The observations started 10:12 UT on 2019 April 25
(about ~1.9 hours after the event) and the median 5 sigma upper limit for
an isolated point source in our images was r > 20.8. No transients were
detected in any of the galaxies listed below:
Name | R.A. | Dec.
------------------------------------------------------------------------
NGC6166 | 16:28:38.23 | 39:33:04.4
NGC4889 | 13:00:08.13 | 27:58:37.2
CB-11.4459 15:18:32.09 | 31:09:40.82
1200-07486009 | 15:12:12.73 | 31:54:36.17
J15122693+3224040
<http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%4012318336&Name=2MASX%20J15122693%2b3224040&submit=submit>
| 15:12:26.92 | 32:24:03.84
J151717.32+304801.3 | 15:17:17.33 | 30:48:01.33
J151303.42+325505.8 | 15:13:03.43 | 32:55:05.81
J15120209+3254551
<http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%402909607&Name=2MASX%20J15120209%2b3254551&submit=submit>
| 15:12:02.07 | 32:54:55.29
J15113637+3142477
<http://simbad.u-strasbg.fr/simbad/sim-id?Ident=%4011050786&Name=2MASX%20J15113637%2b3142477&submit=submit>
| 15:11:36.34 | 31:42:47.31
J151109.81+313833.2 | 15:11:09.82 | 31:38:33.2
The KPED team thanks the National Science Foundation, the National Optical
Astronomical Observatory and the Murty family for support in the building
and operation of KPED.