2021MNRAS.507.1296O


Query : 2021MNRAS.507.1296O

2021MNRAS.507.1296O - Mon. Not. R. Astron. Soc., 507, 1296-1317 (2021/October-2)

Swift/UVOT follow-up of gravitational wave alerts in the O3 era.

OATES S.R., MARSHALL F.E., BREEVELD A.A., KUIN N.P.M., BROWN P.J., DE PASQUALE M., EVANS P.A., FENNEY A.J., GRONWALL C., KENNEA J.A., KLINGLER N.J., PAGE M.J., SIEGEL M.H., TOHUVAVOHU A., AMBROSI E., BARTHELMY S.D., BEARDMORE A.P., BERNARDINI M.G., CAMPANA S., CAPUTO R., CENKO S.B., CUSUMANO G., D'AI A., D'AVANZO P., D'ELIA V., GIOMMI P., HARTMANN D.H., KRIMM H.A., LAHA S., MALESANI D.B., MELANDRI A., NOUSEK J.A., O'BRIEN P.T., OSBORNE J.P., PAGANI C., PAGE K.L., PALMER D.M., PERRI M., RACUSIN J.L., SAKAMOTO T., SBARUFATTI B., SCHLIEDER J.E., TAGLIAFERRI G. and TROJA E.

Abstract (from CDS):

In this paper, we report on the observational performance of the Swift Ultra-violet/Optical Telescope (UVOT) in response to the gravitational wave (GW) alerts announced by the Advanced Laser Interferometer Gravitational Wave Observatory and the Advanced Virgo detector during the O3 period. We provide the observational strategy for follow-up of GW alerts and provide an overview of the processing and analysis of candidate optical/UV sources. For the O3 period, we also provide a statistical overview and report on serendipitous sources discovered by Swift/UVOT. Swift followed 18 GW candidate alerts, with UVOT observing a total of 424 deg2. We found 27 sources that changed in magnitude at the 3σ level compared with archival u- or g-band catalogued values. Swift/UVOT also followed up a further 13 sources reported by other facilities during the O3 period. Using catalogue information, we divided these 40 sources into five initial classifications: 11 candidate active galactic nuclei (AGNs)/quasars, three cataclysmic variables (CVs), nine supernovae, 11 unidentified sources that had archival photometry, and six uncatalogued sources for which no archival photometry was available. We have no strong evidence to identify any of these transients as counterparts to the GW events. The 17 unclassified sources are likely a mix of AGN and a class of fast-evolving transient, and one source may be a CV.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): gravitational waves - ultraviolet: general

Simbad objects: 28

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Number of rows : 28
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 AT 2020cmr SN* 00 32 37.709 +41 18 56.29           SNIIn 4 0
2 AT 2019osy ev 00 55 47.000 -27 04 33.00           ~ 6 0
3 GrW 190814 GWE 00 55.8 -27 05           ~ 433 0
4 AT 2020cja ev 01 48 45.410 +51 25 49.73           ~ 7 0
5 SN 2019wxt SN* 01 55 41.94 +31 25 04.4           ~ 14 0
6 AT 2019wqj ev 02 11 37.08 +34 02 28.8           SNII 4 0
7 GRB 200227A gB 03 45 43.91 +09 28 57.1           ~ 18 0
8 ASASSN -14ha SN* 04 20 01.41 -54 56 17.0           SNII 31 0
9 SN 2019wrt SN* 05 16 47.9971 -07 28 43.354           ~ 4 0
10 AT 2019wrr ev 06 03 39.3447 +60 43 41.682           ~ 3 0
11 ZTF19abanrhr ev 12 49.0 +34 49           ~ 35 0
12 NGC 4993 Sy2 13 09 47.6908761600 -23 23 02.314044636   13.34   11.92   ~ 397 0
13 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
14 SN 2019ebq SN* 17 01 18.339 -07 00 10.52           SNIb/c 11 0
15 SN 2019dzk SN* 17 13 21.95 -09 57 52.1           SNII 7 0
16 SN 2019dzw SN* 17 31 09.96 -08 27 02.6           SNIIn 9 0
17 ZTF19aassfws ev 19 54 40.2867 +61 14 24.044           ~ 2 0
18 AT 2019rpn ev 21 19 41.1993 +37 31 19.460           ~ 2 0
19 AT 2019lvs CV* 21 45 34.903 +20 41 26.12           ~ 4 0
20 GrW 200224 222234 BH ~ ~           ~ 44 0
21 GrW 200115 GWE ~ ~           ~ 160 0
22 GrW 190426 152155 GWE ~ ~           ~ 66 0
23 GrW 191216 213338 GWE ~ ~           ~ 37 0
24 GrW 200225 060421 GWE ~ ~           ~ 35 0
25 GRB 190425 GWE ~ ~           ~ 438 0
26 GrW 190521 GWE ~ ~           ~ 409 0
27 GrW 190412 GWE ~ ~           ~ 169 0
28 GrW 190728 GWE ~ ~           ~ 48 0

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