Binary neutron star merger offsets from their host galaxies - II. Short-duration gamma-ray bursts

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Table A.1.

Sample of SGRB hosts used in this work.

GRB	Host type	z	Offset	M_B	log M_⋆/M_⊙	t_m	τ	R_half	n	$R_{half}^{ms}$ $R_{\mathrm{half}}^{\mathrm{ms}}$	Ref.
			[kpc]			[Gyr]	[Gyr]	[kpc]		[kpc]

Gold sample
050509B	Early	0.22	55.19±12.43	-22.10	11.46	8.84	1.07	20.98	5.60	$6 . 28_{- 0.70}^{+ 7.76}$ $6.28_{-0.70}^{+7.76}$	1,13
050709	Late	0.16	3.760±0.056	-17.63	8.55	0.57	0.10	1.75	0.60	$2 . 10_{- 0.92}^{+ 1.53}$ $2.10_{-0.92}^{+1.53}$	1,13
050724A	Early	0.26	2.74±0.08	-20.42	11.05	8.20	1.07	4.00	2.90	$5 . 30_{- 1.68}^{+ 5.08}$ $5.30_{-1.68}^{+5.08}$	1,13
051221A	Late	0.55	2.08±0.19	-19.91	9.31	0.49	0.14	2.49	0.90	$2 . 79_{- 1.22}^{+ 1.81}$ $2.79_{-1.22}^{+1.81}$	1,13
060614	Late	0.12	0.70±0.79	-15.57	7.85	0.76	0.14	—	—	$1 . 43_{- 0.62}^{+ 1.20}$ $1.43_{-0.62}^{+1.20}$	2,13
060801	Late	1.13	10.25±10.92	-21.19	9.12	0.13	0.48	—	—	$2 . 19_{- 1.00}^{+ 1.58}$ $2.19_{-1.00}^{+1.58}$	3,13
061006	Late	0.46	1.39±0.29	-18.28	9.37	4.27	1.21	3.67	0.70	$3 . 30_{- 1.45}^{+ 1.99}$ $3.30_{-1.45}^{+1.99}$	1,13
061210	Late	0.41	15.51±14.36	-19.41	9.49	0.66	0.11	2.18	1.03	$3 . 53_{- 1.54}^{+ 2.07}$ $3.53_{-1.54}^{+2.07}$	4,13
070429B	Late	0.90	6.00±13.44	-21.54	10.44	0.43	0.11	5.08	2.15	$4 . 81_{- 2.08}^{+ 2.38}$ $4.81_{-2.08}^{+2.38}$	4,13
070714B	Late	0.92	12.33±0.87	-19.74	9.37	1.63	2.07	2.20	1.18	$2 . 89_{- 1.26}^{+ 1.85}$ $2.89_{-1.26}^{+1.85}$	4,13
070724A	Late	0.46	5.52±0.18	-20.76	9.81	0.27	0.10	3.64	0.92	$4 . 13_{- 1.80}^{+ 2.27}$ $4.13_{-1.80}^{+2.27}$	4,13
070809	Early	0.47	34.11±2.75	-21.60	10.82	0.84	0.11	3.38	3.38	$4 . 82_{- 1.98}^{+ 3.94}$ $4.82_{-1.98}^{+3.94}$	4,13
071227A	Late	0.38	14.74±0.26	-19.86	10.79	1.79	0.73	4.72	1.05	$6 . 98_{- 2.76}^{+ 3.56}$ $6.98_{-2.76}^{+3.56}$	4,13
090510	Late	0.90	10.51±2.92	-21.02	9.75	0.45	0.10	7.27^§	1.27^§	$3 . 63_{- 1.54}^{+ 2.12}$ $3.63_{-1.54}^{+2.12}$	4,13
100117A	Late	0.91	1.35±0.32	-20.56	10.35	3.02	0.25	4.95^§	0.55^§	$4 . 59_{- 2.00}^{+ 2.39}$ $4.59_{-2.00}^{+2.39}$	3,4,13
100206A	Late	0.41	25.28±13.05	-20.58	10.72	4.58	3.22	—	—	$6 . 60_{- 2.64}^{+ 3.41}$ $6.60_{-2.64}^{+3.41}$	2,13
101224A	Late	0.45	12.75±13.51	-19.65	9.17	0.46	0.14	—	—	$2 . 96_{- 1.29}^{+ 1.87}$ $2.96_{-1.29}^{+1.87}$	2,13
120804A	Late	1.05^⋆	2.30±1.28	-19.79	9.81	0.35	2.26	—	—	$3 . 10_{- 1.35}^{+ 1.91}$ $3.10_{-1.35}^{+1.91}$	2,13
121226A	Late	1.37^⋆	2.31±9.15	-21.43	9.46	0.12	2.00	—	—	$2 . 61_{- 1.16}^{+ 1.74}$ $2.61_{-1.16}^{+1.74}$	2,13
130603B	Late	0.36	5.4±0.2	-19.86	9.82	1.63	0.37	3.37^§	1.29^§	$4 . 14_{- 1.80}^{+ 2.27}$ $4.14_{-1.80}^{+2.27}$	4,13
140129B	Late	0.43	1.76±1.76	-17.85	9.33	1.65	0.37	—	—	$3 . 23_{- 1.41}^{+ 1.97}$ $3.23_{-1.41}^{+1.97}$	2,13
140903A	Late	0.35	0.9±0.1	-19.22	10.81	4.24	1.09	—	—	$7 . 09_{- 2.79}^{+ 3.61}$ $7.09_{-2.79}^{+3.61}$	2,13
141212A	Late	0.60	18.75±12.29	-19.84	9.71	2.37	1.39	—	—	$3 . 54_{- 1.51}^{+ 2.09}$ $3.54_{-1.51}^{+2.09}$	2,13
150101B	Early	0.13	7.36±0.07	-21.21	11.13	4.88	0.61	9.5	5.0	$5 . 48_{- 1.54}^{+ 5.53}$ $5.48_{-1.54}^{+5.53}$	2,5,13
150120A	Late	0.46	4.77±6.44	-19.74	10.01	2.28	1.21	—	—	$4 . 33_{- 1.86}^{+ 2.37}$ $4.33_{-1.86}^{+2.37}$	2,13
150728A	Late	0.46	7.52±20.29	-20.45	9.35	0.15	0.10	—	—	$3 . 27_{- 1.43}^{+ 1.98}$ $3.27_{-1.43}^{+1.98}$	2,13
160411A	Late	0.81^⋆	1.4±2.3	-18.89	8.87	0.67	2.51	—	—	$2 . 14_{- 0.96}^{+ 1.54}$ $2.14_{-0.96}^{+1.54}$	2,13
160525B	Late	0.64^⋆	5.50±7.38	-18.44	8.04	0.14	2.21	—	—	$1 . 30_{- 0.61}^{+ 1.12}$ $1.30_{-0.61}^{+1.12}$	2,13
170428A	Late	0.45	7.72±3.39	-18.66	9.68	5.14	2.35	—	—	$3 . 92_{- 1.72}^{+ 2.19}$ $3.92_{-1.72}^{+2.19}$	2,13
170728B	Late	1.27	6.76±2.06	-21.99	9.87	0.41	0.34	—	—	$3 . 17_{- 1.38}^{+ 1.95}$ $3.17_{-1.38}^{+1.95}$	2,13
170817A	Early	0.01	2.125±0.001	-19.12	10.61	10.42	1.20	3.3	3.9	$3 . 88_{- 1.70}^{+ 2.80}$ $3.88_{-1.70}^{+2.80}$	6,13
180418A	Late	1.55^⋆	1.30±0.32	-21.20	9.83	0.56	1.67	—	—	$2 . 73_{- 1.22}^{+ 1.85}$ $2.73_{-1.22}^{+1.85}$	7,13
180618A	Late	0.52^⋆	9.70±1.69	-19.51	8.81	0.35	2.47	—	—	$2 . 07_{- 0.93}^{+ 1.51}$ $2.07_{-0.93}^{+1.51}$	2,13
180727A	Late	1.95^⋆	2.56±5.13	-20.48	9.22	0.54	1.75	—	—	$2 . 11_{- 0.95}^{+ 1.56}$ $2.11_{-0.95}^{+1.56}$	2,13
181123B	Late	1.75	5.08±1.38	-22.30	9.90	0.63	1.64	—	—	$2 . 82_{- 1.25}^{+ 1.87}$ $2.82_{-1.25}^{+1.87}$	8,13
200219A	Late	0.48^⋆	8.30±5.28	-20.93	10.74	3.53	2.34	—	—	$6 . 71_{- 2.67}^{+ 3.45}$ $6.71_{-2.67}^{+3.45}$	2,13
200522A	Late	0.55	0.93±0.19	-20.90	9.66	0.58	0.22	3.9	2.1	$3 . 44_{- 1.47}^{+ 2.06}$ $3.44_{-1.47}^{+2.06}$	9,13
200907B	Late	0.56^⋆	2.41±7.78	-19.37	9.35	0.89	1.44	—	—	$2 . 86_{- 1.24}^{+ 1.84}$ $2.86_{-1.24}^{+1.84}$	2,13
210323A	Late	0.73	5.89±3.68	-18.93	8.77	0.56	0.22	—	—	$2 . 02_{- 0.91}^{+ 1.48}$ $2.02_{-0.91}^{+1.48}$	2,13
210726A	Late	0.37^⋆	12.26±2.22	-15.63	7.84	1.06	2.11	—	—	$1 . 42_{- 0.62}^{+ 1.20}$ $1.42_{-0.62}^{+1.20}$	2,13
211023B	Late	0.86	3.84±2.57	-20.02	9.65	1.72	1.15	—	—	$3 . 42_{- 1.46}^{+ 2.05}$ $3.42_{-1.46}^{+2.05}$	2,13
211211A	Late	0.08	7.920±0.029	-17.38	8.84	2.53	0.86	1.64	1	$2 . 46_{- 1.08}^{+ 1.69}$ $2.46_{-1.08}^{+1.69}$	2,10,13

Silver sample
051210	Late	2.58^⋆	29.08±16.34	-24.27	10.96	0.23	1.58	—	—	$3 . 19_{- 1.42}^{+ 2.19}$ $3.19_{-1.42}^{+2.19}$	1,13
070729	Late	0.52^⋆	19.72±14.49	-18.81	8.75	0.55	2.04	—	—	$2 . 00_{- 0.90}^{+ 1.47}$ $2.00_{-0.90}^{+1.47}$	2,13
090515	Early	0.40	76.19±0.16	-20.76	11.25	6.34	0.24	4.24^§	2.95^§	$5 . 75_{- 1.29}^{+ 6.27}$ $5.75_{-1.29}^{+6.27}$	4,13
100625A	Early	0.45	2.63±6.77	-18.84	9.70	3.56	0.21	—	—	$1 . 90_{- 0.81}^{+ 0.98}$ $1.90_{-0.81}^{+0.98}$	2,13
101219A	Late	0.72	5.48±6.65	-19.58	9.39	0.25	0.10	—	—	$2 . 93_{- 1.27}^{+ 1.87}$ $2.93_{-1.27}^{+1.87}$	2,13
111117A	Late	2.21	10.52±1.68	-22.65	9.63	0.19	1.30	—	—	$2 . 13_{- 0.92}^{+ 1.44}$ $2.13_{-0.92}^{+1.44}$	2,13
120305A	Early	0.22	18.09±5.25	-18.25	9.17	2.11	0.38	—	—	$1 . 86_{- 0.79}^{+ 1.03}$ $1.86_{-0.79}^{+1.03}$	2,13

130515A	Early	0.80^⋆	61.22±13.77	-22.09	10.29	0.78	0.10	—	—	$1 . 77_{- 0.67}^{+ 0.97}$ $1.77_{-0.67}^{+0.97}$	2,13
130822A	Early	0.15	60.1±4.9	-20.08	10.16	2.16	0.39	—	—	$2 . 30_{- 1.00}^{+ 1.32}$ $2.30_{-1.00}^{+1.32}$	2,13
140930B	Late	1.46	9.62±4.3	-21.18	9.45	0.57	2.35	—	—	$2 . 59_{- 1.16}^{+ 1.73}$ $2.59_{-1.16}^{+1.73}$	2,13
150831A	Late	1.18	12.21±9.77	-20.43	9.49	0.51	2.00	—	—	$2 . 65_{- 1.18}^{+ 1.75}$ $2.65_{-1.18}^{+1.75}$	2,13
151229A	Late	0.63^⋆	8.16±6.05	-17.27	8.79	1.78	1.37	—	—	$2 . 04_{- 0.92}^{+ 1.49}$ $2.04_{-0.92}^{+1.49}$	2,13
160303A	Late	1.01^⋆	15.3±0.9	-19.29	9.51	1.05	1.52	—	—	$2 . 67_{- 1.19}^{+ 1.76}$ $2.67_{-1.19}^{+1.76}$	2,13
160624A	Late	0.48	9.63±6.24	-19.85	9.74	1.19	0.42	6.8	1	$4 . 05_{- 1.77}^{+ 2.23}$ $4.05_{-1.77}^{+2.23}$	2,12,13
160821B	Late	0.16	15.74±0.03	-19.26	9.24	0.58	0.12	—	—	$3 . 07_{- 1.35}^{+ 1.92}$ $3.07_{-1.35}^{+1.92}$	2,13
161001A	Late	0.67^⋆	18.54±6.22	-20.28	9.73	0.77	0.16	—	—	$3 . 59_{- 1.53}^{+ 2.11}$ $3.59_{-1.53}^{+2.11}$	2,13
161104A	Early	0.79	1.66±16.60	-20.41	10.23	2.26	0.28	—	—	$1 . 70_{- 0.66}^{+ 0.94}$ $1.70_{-0.66}^{+0.94}$	11,13
170127B	Late	2.21^⋆	10.37±13.60	-21.80	9.51	0.31	1.69	—	—	$2 . 03_{- 0.86}^{+ 1.41}$ $2.03_{-0.86}^{+1.41}$	2,13
180805B	Late	0.66	24.30±7.49	-20.17	9.34	0.50	0.22	—	—	$2 . 84_{- 1.24}^{+ 1.83}$ $2.84_{-1.24}^{+1.83}$	2,13
191031D	Late	1.93^⋆	13.08±10.69	-22.32	10.38	0.80	1.43	—	—	$3 . 49_{- 1.51}^{+ 2.01}$ $3.49_{-1.51}^{+2.01}$	2,13

Bronze sample
050813	Late	0.72	43.57±17.37	-20.29	10.31	3.73	1.30	—	—	$4 . 50_{- 1.96}^{+ 2.39}$ $4.50_{-1.96}^{+2.39}$	2,13
080123	Late	0.50	53.63±7.67	-20.89	10.12	0.43	0.29	—	—	$4 . 16_{- 1.81}^{+ 2.32}$ $4.16_{-1.81}^{+2.32}$	2,13
140622A	Late	0.96	32.95±11.25	-21.80	10.17	0.66	0.24	—	—	$4 . 24_{- 1.85}^{+ 2.35}$ $4.24_{-1.85}^{+2.35}$	2,13
160408A	Late	1.91^⋆	14.13±1.25	-20.88	9.32	0.62	1.84	—	—	$2 . 20_{- 0.99}^{+ 1.61}$ $2.20_{-0.99}^{+1.61}$	2,13
170728A	Late	1.49	32.25±3.01	-19.85	10.09	0.16	2.07	—	—	$3 . 48_{- 1.49}^{+ 2.07}$ $3.48_{-1.49}^{+2.07}$	2,13
200411A	Late	0.83^⋆	41.98±7.48	-21.53	10.23	0.62	2.99	—	—	$4 . 33_{- 1.89}^{+ 2.38}$ $4.33_{-1.89}^{+2.38}$	2,13
201221D	Late	1.06	29.35±24.09	-20.96	9.36	0.27	0.10	—	—	$2 . 48_{- 1.11}^{+ 1.69}$ $2.48_{-1.11}^{+1.69}$	2,13
210919A	Late	0.24	51.05±1.92	-19.42	9.87	1.62	0.32	—	—	$4 . 19_{- 1.82}^{+ 2.30}$ $4.19_{-1.82}^{+2.30}$	2,13

Notes. The columns list the gamma-ray burst name, the host galaxy type, the host redshift, the projected offset, the rest-frame total magnitude in the B band, the stellar mass, the mass-weighted age, the scale age, the observed half-light radius, the observed Sérsic index, the half-light radius from the mass-size relation, and the references for the listed values. ^( ⋆ )Photometric redshift inferred from SED fitting by Nugent et al. (2022). $^{(§)}$ $^{(\S)}$ Sérsic profile of the dominant component.

References. (1) Fong et al. (2010); (2) Fong et al. (2022); (3) Berger et al. (2007); (4) Fong & Berger (2013); (5) Fong et al. (2016); (6) Blanchard et al. (2017); (7) Rouco Escorial et al. (2021); (8) Paterson et al. (2020); (9) Fong et al. (2021); (10) Rastinejad et al. (2022); (11) Nugent et al. (2020); (12) O’Connor et al. (2021); (13) Nugent et al. (2022).

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