2022ApJS..261...25D

Query : 2022ApJS..261...25D

2022ApJS..261...25D - Astrophys. J., Suppl. Ser., 261, 25 (2022/August-1)

The Optical Two- and Three-dimensional Fundamental Plane Correlations for Nearly 180 Gamma-Ray Burst Afterglows with Swift/UVOT, RATIR, and the Subaru Telescope.

DAINOTTI M.G., YOUNG S., LI L., LEVINE D., KALINOWSKI K.K., KANN D.A., TRAN B., ZAMBRANO-TAPIA L., ZAMBRANO-TAPIA A., CENKO S.B., FUENTES M., SANCHEZ-VAZQUEZ E.G., OATES S.R., FRAIJA N., BECERRA R.L., WATSON A.M., BUTLER N.R., GONZALEZ J.J., KUTYREV A.S., LEE W.H., PROCHASKA J.X., RAMIREZ-RUIZ E., RICHER M.G. and ZOLA S.

Abstract (from CDS):

Gamma-ray bursts (GRBs) are fascinating events due to their panchromatic nature. We study optical plateaus in GRB afterglows via an extended search into archival data. We comprehensively analyze all published GRBs with known redshifts and optical plateaus observed by many ground-based telescopes (e.g., Subaru Telescope, RATIR) around the world and several space-based observatories such as the Neil Gehrels Swift Observatory. We fit 500 optical light curves, showing the existence of the plateau in 179 cases. This sample is 75% larger than the previous one, and it is the largest compilation so far of optical plateaus. We discover the 3D fundamental plane relation at optical wavelengths using this sample. This correlation is between the rest-frame time at the end of the plateau emission, ${T}_{\mathrm{opt}}^{* }$, its optical luminosity, Lopt, and the peak in the optical prompt emission, Lpeak,opt, thus resembling the three-dimensional (3D) X-ray fundamental plane (the so-called 3D Dainotti relation). We correct our sample for redshift evolution and selection effects, discovering that this correlation is indeed intrinsic to GRB physics. We investigate the rest-frame end-time distributions in X-rays and optical (${T}_{\mathrm{opt}}^{* }$, ${T}_{{\rm{X}}}^{* }$), and conclude that the plateau is achromatic only when selection biases are not considered. We also investigate if the 3D optical correlation may be a new discriminant between optical GRB classes and find that there is no significant separation between the classes compared to the Gold sample plane after correcting for evolution.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Gamma-ray bursts ;

VizieR on-line data: <Available at CDS (J/ApJS/261/25): table1.dat refs.dat>

Simbad objects: 185

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Number of rows : 185
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 070110 gB 00 03 39.270 -52 58 27.00 21.8 21.9 21.2     ~ 220 0
3 GRB 150910A gB 00 22 40.14 +33 28 22.4           ~ 79 0
4 GRB 071031 gB 00 25 37.40 -58 03 33.9           ~ 184 0
5 GRB 021004 gB 00 26 54.68 +18 55 41.6           ~ 560 0
6 GRB 170607A gB 00 29 27.84 +09 14 35.5           ~ 62 0
7 GRB 060708 gB 00 31 13.850 -33 45 32.40 19.07 19.79 17.37     ~ 109 0
8 GRB 080710 gB 00 33 05.68 +19 30 05.8           ~ 136 0
9 GRB 180115A gB 00 48 09.31 -15 37 50.5           ~ 28 0
10 SN 2010ma SN* 00 48 55.35 -34 33 59.5           SNIc 190 1
11 GRB 050824 gB 00 48 56.100 +22 36 32.00 19.66 21.03 20.46 23.70   ~ 184 0
12 GRB 201021C gB 00 50 06.93 -55 51 55.8           ~ 21 0
13 Fermi bn120729456 gB 00 52 17.84 +49 56 23.1           ~ 122 0
14 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
15 GRB 041006 gB 00 54 50.17 +01 14 07.0           ~ 202 2
16 GRB 050904 gB 00 54 50.794 +14 05 09.42           ~ 496 0
17 SN 2011kl SN* 00 57 22.64 -46 48 03.6           SNSLSN 268 1
18 GRB 050908 gB 01 21 50.750 -12 57 17.20           ~ 179 0
19 GRB 201014A gB 01 23 11.09 +27 39 36.9           ~ 18 0
20 Fermi bn100814160 gB 01 29 53.61 -17 59 43.6           ~ 219 0
21 GRB 051028 gB 01 48 15.010 +47 45 09.20           ~ 39 0
22 GRB 100901A gB 01 49 03.56 +22 45 30.6           ~ 170 0
23 GRB 100906A gB 01 54 44.19 +55 37 49.8           ~ 233 0
24 GRB 040924 gB 02 06 22.52 +16 08 48.8           ~ 169 1
25 GRB 091018 gB 02 08 46 -57 33.0           ~ 169 0
26 GRB 170714A gB 02 17 17 +01 58.0           ~ 50 0
27 SN 2009nz SN* 02 26 19.87 -18 57 08.6           ~ 307 1
28 GRB 151029A gB 02 34 06.71 -35 23 07.8           ~ 40 0
29 GRB 071112C gB 02 36 50.89 +28 22 16.9           ~ 164 0
30 GRB 081228 gB 02 37 50.80 +30 51 09.2           ~ 43 0
31 GRB 050603 gB 02 39 56.839 -25 10 54.92     18.48     ~ 174 0
32 Fermi bn110213220 gB 02 51 51.37 +49 16 21.2           ~ 175 0
33 SN 2013ez SN* 02 53 56.70 +13 23 13.6           ~ 118 0
34 GRB 140801A gB 02 56 16.50 +30 56 16.8           ~ 55 0
35 GRB 191011A gB 02 58 54.70 -27 50 43.4           ~ 38 0
36 GRB 061007 gB 03 05 19.510 -50 30 02.50 14.28 14.40 12.95     ~ 315 1
37 GRB 140907A gB 03 12 34.98 +46 36 17.2           ~ 81 0
38 GRB 070318 gB 03 13 56.830 -42 56 46.30 18.27 16.23 15.49     ~ 170 0
39 GRB 050318 gB 03 18 51.000 -46 23 43.61 18.10 18.68 17.58     ~ 189 0
40 GRB 181010A gB 03 30 16.88 -23 02 17.9           ~ 39 0
41 GRB 060210 gB 03 50 57.370 +27 01 34.40   20.27       ~ 275 0
42 GRB 060904B gB 03 52 50.520 -00 43 30.61 18.27 19.14 18.37     ~ 208 0
43 GRB 091029 gB 04 00 40.00 -55 57 12.7           ~ 168 0
44 Fermi bn170113420 gB 04 06 59 -71 56.0           ~ 64 0
45 GRB 080913 gB 04 22 57.90 -25 07 38.6           ~ 213 0
46 GRB 060313 G 04 26 28.4020 -10 50 39.901 20.55 21.03 19.66     ~ 156 0
47 Fermi bn120907017 gB 04 58 59.99 -09 18 53.7           ~ 89 0
48 GRB 100508A gB 05 04 58.99 -20 42 14.1           ~ 39 0
49 GRB 060124 gB 05 08 25.900 +69 44 26.98   18.91 17.35     ~ 280 0
50 GRB 160131A gB 05 12 40.31 -07 02 59.4           ~ 86 0
51 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
52 GRB 061126 gB 05 46 24.460 +64 12 38.49 18.62 18.79 19.20     ~ 182 1
53 GRB 110801A gB 05 57 44.87 +80 57 21.1           ~ 90 0
54 SN 2016jca SN* 06 06 51.36 -26 47 29.7           SNIc 140 0
55 Fermi bn120711115 gB 06 18 42.839 -70 59 56.78           ~ 125 0
56 Fermi bn080928628 gB 06 20 16.85 -55 11 59.3           ~ 187 0
57 GRB 060729 gB 06 21 31.850 -62 22 12.69           ~ 303 0
58 GRB 140430A gB 06 51 44.58 +23 01 25.5           ~ 81 0
59 GRB 970508 gB 06 53 49.2 +79 16 19           ~ 883 1
60 GRB 070411 gB 07 09 19.930 +01 03 52.60     17.94     ~ 138 0
61 SN 2010bh SN* 07 10 30.63 -56 15 19.7           SNIc 336 1
62 GRB 110422A gB 07 28 11.21 +75 06 24.0           ~ 113 0
63 GRB 160314A gB 07 31 09.80 +16 59 57.5           ~ 38 0
64 GRB 210204A gB 07 48 19.37 +11 24 34.2           ~ 46 0
65 GRB 070125 gB 07 51 17.80 +31 09 04.8           ~ 188 0
66 Fermi bn120119170 gB 08 00 06.940 -09 04 53.83           ~ 193 0
67 GRB 070612A gB 08 05 28.530 +37 16 09.57           ~ 82 0
68 GRB 141121A gB 08 10 40.68 +22 13 02.7           ~ 108 0
69 Fermi bn180205184 gB 08 27 16.72 +11 32 32.6           ~ 60 0
70 GRB 150323A gB 08 32 42.73 +45 27 52.9           ~ 68 0
71 GRB 090102 gB 08 32 59.50 +33 06 25.7           ~ 253 0
72 GRB 980326 gB 08 36 34.3 -18 51 24           ~ 268 0
73 Fermi bn111107035 gB 08 37 54.66 -66 31 12.3           ~ 97 0
74 GRB 110503A gB 08 51 06.31 +52 12 27.7           ~ 115 0
75 GRB 050502B gB 09 30 10.024 +16 59 48.07           ~ 169 0
76 GRB 020124 gB 09 32 50.8 -11 31 11           ~ 155 0
77 GRB 061021 gB 09 40 36.120 -21 57 05.40 18.21 19.20 16.82     ~ 160 0
78 Fermi bn140206304 gB 09 41 16.90 +66 45 42.7           ~ 149 0
79 GRB 061121 gB 09 48 54.570 -13 11 42.68 17.19 17.71 17.02     ~ 350 0
80 Fermi bn090423330 gB 09 55 33.19 +18 08 57.7           ~ 392 0
81 Fermi bn111228657 gB 10 00 16.04 +18 17 52.2           ~ 201 0
82 GRB 071010B gB 10 02 09.20 +45 43 52.2           ~ 173 0
83 GRB 200613A gB 10 12 10.03 +45 45 14.1           ~ 36 0
84 Fermi bn121217313 gB 10 14 50.32 -62 21 03.3           ~ 69 0
85 GRB 050319 gB 10 16 47.900 +43 32 53.80   18.02 17.01     ~ 274 0
86 GRB 100219A gB 10 16 48.48 -12 34 00.0           ~ 130 0
87 GRB 180325A gB 10 29 42.57 +24 27 48.7           ~ 85 0
88 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
89 GRB 100316B gB 10 54 00 -45 28.0           ~ 62 0
90 GRB 110205A gB 10 58 31.12 +67 31 31.2           ~ 213 0
91 GRB 011211 gB 11 15 16 -21 56.0           ~ 305 0
92 GRB 080330 gB 11 17 06.70 +30 36 24.1           ~ 145 0
93 GRB 100513A gB 11 18 26.83 +03 37 40.8           ~ 74 0
94 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 613 1
95 GRB 030226 gB 11 33 04.9 +25 53 56           ~ 212 0
96 Fermi bn091020900 gB 11 42 55.20 +50 58 42.0           ~ 188 0
97 GRB 080603B gB 11 46 07.46 +68 03 38.5           ~ 153 0
98 GRB 090530 gB 11 57 36.00 +26 35 23.0           ~ 89 0
99 GRB 050408 gB 12 02 17.320 +10 51 10.00           ~ 153 0
100 GRB 030328 gB 12 10 48.4 -09 20 51           ~ 148 0
101 GRB 070419A gB 12 10 58.830 +39 55 34.06 18.52         ~ 130 0
102 GRB 030429 gB 12 13 07.495 -20 54 49.54     23.70     ~ 132 0
103 GRB 050416 gB 12 33 54.600 +21 03 26.69     19.12     ~ 300 1
104 GRB 090426 G 12 36 18.0470 +32 59 09.460           ~ 237 0
105 GRB 070810A gB 12 39 51.18 +10 45 02.8           ~ 80 0
106 GRB 150413A gB 12 41 35.10 +71 50 21.9           ~ 70 0
107 GRB 160227A gB 12 59 13.71 +78 40 45.1           ~ 69 0
108 GRB 080607A gB 12 59 47.14 +15 55 09.6           ~ 257 0
109 GRB 060512 gB 13 03 05.810 +41 11 27.21 19.12 19.63 17.20     ~ 142 0
110 Fermi bn130420313 gB 13 04 25.49 +59 25 26.8           ~ 112 0
111 Fermi bn140423356 gB 13 09 06.20 +49 50 18.3           ~ 114 0
112 GRB 070208 gB 13 11 32.607 +61 57 54.37 20.79 20.79 19.86     ~ 119 0
113 Fermi bn141221338 gB 13 13 09.02 +08 12 18.3           ~ 76 0
114 GRB 090313 gB 13 13 36.00 +08 05 10.7           ~ 149 0
115 GRB 050502A gB 13 29 46.250 +42 40 27.50           ~ 65 0
116 GRB 060206 gB 13 31 43.420 +35 03 03.60   19.99 17.09     ~ 330 0
117 GRB 050801 gB 13 36 35.000 -21 55 41.00 15.03 15.82 15.46     ~ 164 0
118 GRB 990510 gB 13 38 07.64 -80 29 48.8           ~ 499 1
119 GRB 050730 gB 14 08 17.090 -03 46 18.90   20.32 17.68     ~ 327 0
120 GRB 090529A gB 14 09 52.56 +24 27 32.2           ~ 23 0
121 SN 2013dx SN* 14 29 14.77 +15 46 26.6           ~ 178 0
122 GRB 050802 gB 14 37 05.820 +27 47 12.62 16.85 17.38 16.97     ~ 186 0
123 Fermi bn170405777 gB 14 39 18.66 -25 14 36.9           ~ 75 0
124 GRB 080310 gB 14 40 13.89 -00 10 30.4           ~ 214 0
125 Fermi bn160804065 gB 14 46 31.20 +09 59 56.1           ~ 79 0
126 GRB 010222 G 14 52 12.5 +43 01 06           ~ 364 1
127 GRB 060714 gB 15 11 26.450 -06 33 58.30   20.21 18.54     ~ 209 0
128 GRB 060526 gB 15 31 18.360 +00 17 04.90   18.31 17.16     ~ 288 0
129 GRB 081203A gB 15 32 07.6 +63 31 15           ~ 177 0
130 GRB 120404A gB 15 40 02.29 +12 53 06.3           ~ 104 0
131 GRB 060418 gB 15 45 42.600 -03 38 20.00 15.73 16.19 14.98     ~ 389 0
132 GRB 110715A gB 15 50 44.090 -46 14 06.53           ~ 120 0
133 GRB 190627A gB 16 19 18.73 -05 17 20.4           ~ 43 0
134 GRB 000301C gB 16 20 18.5 +29 26 35           ~ 361 0
135 GRB 050401 gB 16 31 28.84 +02 11 14.5           ~ 348 0
136 GRB 090726 gB 16 34 43.50 +72 51 56.5           ~ 70 0
137 GRB 130606A gB 16 37 35.12 +29 47 46.4           ~ 185 0
138 GRB 200829A gB 16 44 49.42 +72 19 45.3           ~ 55 0
139 GRB 000926 gB 17 04 15 +51 46.0           ~ 373 0
140 GRB 100418A gB 17 05 26.96 +11 27 41.9           ~ 198 0
141 GRB 080319C gB 17 15 55.48 +55 23 31.7           ~ 174 0
142 GRB 201020A gB 17 24 54.73 +31 25 41.7           ~ 30 0
143 GRB 080605 gB 17 28 30.04 +04 00 56.9           ~ 198 0
144 GRB 210210A gB 17 31 04.90 +14 39 45.1           ~ 30 0
145 Fermi bn151027166 gB 18 09 56.87 +61 21 12.3           ~ 143 0
146 GRB 120815A gB 18 15 54.40 -52 07 29.0           ~ 103 0
147 SN 2005nc SN* 18 32 32.560 +26 20 22.34           SNIc: 400 1
148 GRB 080603A gB 18 37 37.95 +62 44 39.6           ~ 89 0
149 Fermi bn081008832 gB 18 39 52.40 -57 25 58.8           ~ 224 0
150 GRB 160425A gB 18 41 18.56 -54 21 36.1           ~ 49 0
151 Fermi bn110731465 gB 18 42 00.99 -28 32 13.8           ~ 193 0
152 GRB 110726A gB 19 06 52.21 +56 04 16.4           ~ 55 0
153 GRB 080413A gB 19 09 11.73 -27 40 39.6           ~ 163 0
154 GRB 071010A gB 19 12 14.42 -32 24 06.2           ~ 138 0
155 GRB 060413 gB 19 25 07.850 +13 45 29.90           ~ 69 0
156 GRB 090618 gB 19 36 01.80 +78 21 07.1           ~ 358 0
157 Fermi bn121128212 gB 20 02 23.88 +54 17 59.1           ~ 128 0
158 GRB 071003A gB 20 07 25 +10 56.9           ~ 7 0
159 GRB 120923A gB 20 15 10.73 +06 13 16.9           ~ 59 0
160 GRB 161023A gB 20 44 05.20 -47 39 48.7           ~ 49 0
161 GRB 100621A gB 21 01 13.12 -51 06 22.5           ~ 204 0
162 GRB 050922C gB 21 09 33.000 -08 45 30.10 15.15 15.86 14.69     ~ 301 0
163 GRB 181201A gB 21 17 11.20 -12 37 50.9           ~ 60 0
164 GRB 060614 G 21 23 32.140 -53 01 36.10           ~ 714 0
165 GRB 060605 gB 21 28 37.320 -06 03 31.30   20.12 16.53     ~ 210 0
166 GRB 060522 gB 21 31 44.850 +02 53 10.80           ~ 140 0
167 GRB 080413B gB 21 44 34.62 -19 58 51.2           ~ 191 0
168 GRB 060927A gB 21 58 11.930 +05 21 50.32           ~ 215 0
169 GRB 060607 gB 21 58 50.400 -22 29 46.70 18.49 16.67 15.09     ~ 318 0
170 GRB 051109A gB 22 01 15.320 +40 49 23.70   20.09 20.14     ~ 190 0
171 Fermi bn081109293 gB 22 03 11.50 -54 42 40.5           ~ 125 1
172 GRB 060505 gB 22 07 03.440 -27 48 51.89           ~ 286 1
173 GRB 161014A gB 22 10 35.42 +07 28 07.6           ~ 69 0
174 Fermi bn090510016 G 22 14 12.6230 -26 34 58.550           ~ 548 0
175 GRB 050820A gB 22 29 38.110 +19 33 37.10 18.33 19.00 18.47     ~ 409 0
176 Fermi bn091024380 gB 22 37 +56.9           ~ 151 0
177 SN 2008hw SN* 22 39 50.39 -40 08 49.1           SNIc 197 1
178 GRB 170604A gB 22 50 37.49 -15 24 44.6           ~ 37 0
179 Fermi bn090927422 gB 22 55 53.41 -70 58 49.3           ~ 112 0
180 GRB 081029A gB 23 07 05.35 -68 09 19.8           ~ 5 0
181 GRB 051111A gB 23 12 33.170 +18 22 28.80 19.77 20.08 19.50     ~ 223 0
182 GRB 201015A gB 23 37 16.43 +53 24 57.6           ~ 74 0
183 GRB 071025 gB 23 40 17.02 +31 46 42.4           ~ 122 0
184 Fermi bn080810549 gB 23 47 08.00 +00 18 35.1           ~ 240 0
185 SN 2013fu SN* 23 54 29.91 +29 25 47.6           SNIb/c 144 1

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