Table 8.
Parameters obtained from the literature and by our SED fitting to archival photometric data using the BAGPIPES package (Carnall et al. 2018).
FXRT | ID | RA (deg) | Dec (deg) | Offset | z or d(Mpc) | Log(Age/yr) | Log(M*/M⊙) | Log(SFR/(M⊙/yr)) | AV (mag) | References |
---|---|---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
Parameters obtained from the literature | ||||||||||
1 | XRT 000519 (†) | 186.54893 | 12.94622 | 12![]() |
16.4 | – | 11.89 | −2.0 | 0.081 | 1,15 |
2 | XRT 010908 | 167.87904 | 55.67411 | 0![]() |
9.3 | – | 11.11 | 0.34 | 0.046 | 2,3,13,14 |
3 | XRT 070530 | 201.36506 | −43.01911 | 5![]() |
4.04 | – | 11.0 | 0.0 | 0.315 | 4,5,13,16 |
4 | XRT 071203 | 211.25671 | 53.66222 | 0![]() |
6.9 | – | 8.87 | −1.15 | 0.029 | 6,7,13,17 |
5 | XRT 080331 | 170.06235 | 12.99154 | 1![]() |
8.1 | – | 10.80 | 0.51 | 0.091 | 8,9,13,14 |
6 | XRT 130822 | 345.50403 | 15.96478 | 1![]() |
29.3 | – | 10.40 | 0.14 | 0.211 | 10,11,13 |
14 | XRT 141001 | 53.16158 | −27.85938 | 0![]() |
2.23![]() |
– | 7.99 | 0.06 | 0.021 | 12,18 |
Parameters derived from photometric data using BAGPIPES (Carnall et al. 2018) | ||||||||||
8 | XRT 041230 | 318.12653 | −63.49895 | 0![]() |
0.61![]() |
9.6![]() |
10.5![]() |
![]() |
0.9![]() |
– |
9 | XRT 080819 | 175.00511 | −31.91749 | 0![]() |
0.7![]() |
8.2![]() |
10.4![]() |
2.1![]() |
1.6![]() |
– |
Notes. Column 1: FXRT candidate number. Column 2: Candidate ID. Column 3 and 4: Right ascension and declination of the host galaxies. Column 5: Angular offset between the transient and the host galaxy. Column 6: Host galaxy redshift or distance. Columns 7, 8, 9: Logarithmic values of the age of the stellar population, the stellar mass, and the SFR from the host galaxies. Column 10: Dust attenuation. Column 11: Literature references.
References. (1) Rhode et al. (2007), (2) Wiegert et al. (2015), (3) Rhode et al. (2007), (4) Espada et al. (2019), (5) Rejkuba et al. (2011), (6) Drozdovsky & Karachentsev (2000), (7) Lanz et al. (2013), (8) Buta et al. (2015), (9) Beuther et al. (2017), (10) Cappellari et al. (2011), (11) Davis et al. (2014), (12) Bauer et al. (2017), (13) Helou et al. (1991), (14) Sorce et al. (2014), (15) Jonker et al. (2013), (16) Crnojević et al. (2016), (17) Tully et al. (2013), (18) Schlafly & Finkbeiner (2011).
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