2024MNRAS.533.4023D


Query : 2024MNRAS.533.4023D

2024MNRAS.533.4023D - Mon. Not. R. Astron. Soc., 533, 4023-4043 (2024/October-1)

An optical gamma-ray burst catalogue with measured redshift - I. Data release of 535 gamma-ray bursts and colour evolution.

DAINOTTI M.G., DE SIMONE B., MOHIDEEN MALIK R.F., PASUMARTI V., LEVINE D., SAHA N., GENDRE B., KIDO D., WATSON A.M., BECERRA R.L., BELKIN S., DESAI S., DO ESPIRITO SANTO PEDREIRA A.C.C., DAS U., LI L., OATES S.R., CENKO S.B., POZANENKO A., VOLNOVA A., HU Y.-D., CASTRO-TIRADO A.J., ORANGE N.B., MORIYA T.J., FRAIJA N., NIINO Y., RINALDI E., BUTLER N.R., GONZALEZ J.D.J.G., KUTYREV A.S., LEE W.H., PROCHASKA X., RAMIREZ-RUIZ E., RICHER M., SIEGEL M.H., MISRA K., ROSSI A., LOPRESTI C., QUADRI U., STRABLA L., RUOCCO N., LEONINI S., CONTI M., ROSI P., RAMIREZ L.M.T., ZOLA S., JINDAL I., KUMAR R., CHAN L., FUENTES M., LAMBIASE G., KALINOWSKI K.K. and JAMAL W.

Abstract (from CDS):

We present the largest optical photometry compilation of gamma-ray bursts (GRBs) with redshifts (z). We include 64813 observations of 535 events (including upper limits) from 28 February 1997 to 18 August 2023. We also present a user-friendly web tool grbLC which allows users to visualize photometry, coordinates, redshift, host galaxy extinction, and spectral indices for each event in our database. Furthermore, we have added a Gamma-ray Coordinate Network (GCN) scraper that can be used to collect data by gathering magnitudes from the GCNs. The web tool also includes a package for uniformly investigating colour evolution. We compute the optical spectral indices for 138 GRBs, for which we have at least four filters at the same epoch in our sample, and craft a procedure to distinguish between GRBs with and without colour evolution. By providing a uniform format and repository for the optical catalogue, this web-based archive is the first step towards unifying several community efforts to gather the photometric information for all GRBs with known redshifts. This catalogue will enable population studies by providing light curves (LCs) with better coverage since we have gathered data from different ground-based locations. Consequently, these LCs can be used to train future LC reconstructions for an extended inference of the redshift. The data gathering also allows us to fill some of the orbital gaps from Swift in crucial points of the LCs, e.g. at the end of the plateau emission or where a jet break is identified.

Abstract Copyright: © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): catalogue - gamma-ray burst: individual

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 74

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Number of rows : 74
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 GRB 101225A gB 00 00 47.48 +44 36 01.0           ~ 163 0
2 GRB 150910A gB 00 22 40.14 +33 28 22.4           ~ 79 0
3 GRB 071031 gB 00 25 37.40 -58 03 33.9           ~ 184 0
4 GRB 021004 gB 00 26 54.68 +18 55 41.6           ~ 560 0
5 SN 2010ma SN* 00 48 55.35 -34 33 59.5           SNIc 190 1
6 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
7 GRB 041006 gB 00 54 50.17 +01 14 07.0           ~ 202 2
8 Fermi bn100814160 gB 01 29 53.61 -17 59 43.6           ~ 219 0
9 GRB 091018 gB 02 08 46 -57 33.0           ~ 169 0
10 GRB 000911 gB 02 18 42 +07 48.0           ~ 163 0
11 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
12 GRB 181010A gB 03 30 16.88 -23 02 17.9           ~ 39 0
13 GRB 171010A gB 04 26 19.41 -10 27 47.9           SNIc-BL 109 0
14 GRB 970228 gB 05 01 46.7 +11 46 53           ~ 650 1
15 Fermi bn141004973 gB 05 06 56.11 +12 49 10.1           ~ 75 0
16 GRB 060124 gB 05 08 25.900 +69 44 26.98   18.91 17.35     ~ 280 0
17 GRB 160131A gB 05 12 40.31 -07 02 59.4           ~ 86 0
18 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
19 GRB 061126 gB 05 46 24.460 +64 12 38.49 18.62 18.79 19.20     ~ 182 1
20 SN 2016jca SN* 06 06 51.36 -26 47 29.7           SNIc 140 0
21 Fermi bn080928628 gB 06 20 16.85 -55 11 59.3           ~ 187 0
22 GRB 080109 gB 06 31 29.0 +70 37 14           ~ 36 0
23 GRB 970508 gB 06 53 49.2 +79 16 19           ~ 883 1
24 SN 2010bh SN* 07 10 30.63 -56 15 19.7           SNIc 336 1
25 GRB 160121A gB 07 16 21.15 -23 35 31.8           ~ 41 0
26 Fermi bn120119170 gB 08 00 06.940 -09 04 53.83           ~ 193 0
27 GRB 081028 gB 08 07 34.40 +02 18 16.8           ~ 125 0
28 GRB 150323A gB 08 32 42.73 +45 27 52.9           ~ 68 0
29 GRB 110503A gB 08 51 06.31 +52 12 27.7           ~ 115 0
30 SN 2012bz SN* 09 07 38.38 +14 01 07.5           SNIb/c 193 1
31 Fermi bn161017745 gB 09 31 04.53 +43 07 35.0           ~ 75 0
32 Fermi bn111228657 gB 10 00 16.04 +18 17 52.2           ~ 201 0
33 GRB 170202A gB 10 10 06 +05 01.0           ~ 90 0
34 GRB 050319 gB 10 16 47.900 +43 32 53.80   18.02 17.01     ~ 274 0
35 GRB 180325A gB 10 29 42.57 +24 27 48.7           ~ 85 0
36 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
37 GRB 110205A gB 10 58 31.12 +67 31 31.2           ~ 213 0
38 GRB 080430 gB 11 01 14.63 +51 41 07.8           ~ 157 0
39 GRB 030323 gB 11 06 09.4 -21 46 13           ~ 138 1
40 SN 2017iuk SN* 11 09 39.49 -12 35 18.7           SNII 210 0
41 GRB 080330 gB 11 17 06.70 +30 36 24.1           ~ 145 0
42 Fermi bn180418281 G 11 20 29.2100 +24 55 58.734           ~ 57 0
43 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 613 1
44 GRB 011121 gB 11 34 26.67 -76 01 41.6       23.0   ~ 286 1
45 Fermi bn141220252 gB 13 00 15.70 +32 08 47.2           ~ 81 0
46 Fermi bn141221338 gB 13 13 09.02 +08 12 18.3           ~ 76 0
47 GRB 090313 gB 13 13 36.00 +08 05 10.7           ~ 149 0
48 GRB 990510 gB 13 38 07.64 -80 29 48.8           ~ 499 1
49 SN 2013dx SN* 14 29 14.77 +15 46 26.6           ~ 178 0
50 GRB 080319B gB 14 31 41.04 +36 18 09.2           ~ 508 0
51 GRB 010222 G 14 52 12.5 +43 01 06           ~ 364 1
52 GRB 210610B gB 16 15 40.47 +14 23 56.3           ~ 87 0
53 GRB 991208 gB 16 33 53.51 +46 27 21.5           ~ 269 1
54 GRB 230812B gB 16 36 31.49 +47 51 31.3           ~ 89 0
55 GRB 200829A gB 16 44 49.42 +72 19 45.3           ~ 55 0
56 GRB 100418A gB 17 05 26.96 +11 27 41.9           ~ 198 0
57 GRB 080605 gB 17 28 30.04 +04 00 56.9           ~ 198 0
58 * alf Lyr dS* 18 36 56.33635 +38 47 01.2802 0.03 0.03 0.03 0.07 0.10 A0V 2787 1
59 Fermi bn160821937 gB 18 39 54.550 +62 23 30.35           ~ 190 0
60 GRB 071010A gB 19 12 14.42 -32 24 06.2           ~ 138 0
61 GRB 221009A gB 19 13 03.85 +19 46 22.7           ~ 433 0
62 GRB 210731A gB 20 01 13.13 -28 03 39.7           ~ 28 0
63 GRB 071003A gB 20 07 25 +10 56.9           ~ 7 0
64 GRB 161023A gB 20 44 05.20 -47 39 48.7           ~ 49 0
65 GRB 100621A gB 21 01 13.12 -51 06 22.5           ~ 204 0
66 GRB 210619B gB 21 18 52.39 +33 51 00.2           ~ 93 0
67 GRB 141028A gB 21 30 24.46 -00 13 55.6           ~ 109 0
68 GRB 080413B gB 21 44 34.62 -19 58 51.2           ~ 191 0
69 iPTF 14bfu SN* 21 52 30.00 +32 00 52.5           SNIc 80 0
70 Fermi bn090510016 G 22 14 12.6230 -26 34 58.550           ~ 548 0
71 GRB 081029A gB 23 07 05.35 -68 09 19.8           ~ 5 0
72 Fermi bn090926181 gB 23 33 36.18 -66 19 25.9           ~ 339 0
73 GRB 201015A gB 23 37 16.43 +53 24 57.6           ~ 74 0
74 GRB 071025 gB 23 40 17.02 +31 46 42.4           ~ 122 0

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