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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 122 16.4 11.89 −2.0 0.081 1,15
2 XRT 010908 167.87904 55.67411 04 9.3 11.11 0.34 0.046 2,3,13,14
3 XRT 070530 201.36506 −43.01911 55 4.04 11.0 0.0 0.315 4,5,13,16
4 XRT 071203 211.25671 53.66222 04 6.9 8.87 −1.15 0.029 6,7,13,17
5 XRT 080331 170.06235 12.99154 13 8.1 10.80 0.51 0.091 8,9,13,14
6 XRT 130822 345.50403 15.96478 12 29.3 10.40 0.14 0.211 10,11,13
14 XRT 141001 53.16158 −27.85938 013 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 07 0.61 9.6 10.5 0.9
9 XRT 080819 175.00511 −31.91749 05 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.

(†)

Assuming the FXRT is associated with galaxy M86.

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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