Table 3.
Properties of the extragalactic FXT candidates detected and/or discussed in this work, ordered by date.
FXT | Id | ObId | Exp. (ks) | Date | T90 (ks) | RA (deg) | Dec (deg) | Off. ang. | Pos. unc. | HR | S/N |
---|---|---|---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
15 | XRT 140507 | 16093 | 68.8 | 2014-05-07 | 4.8![]() |
233.73496 | 23.46849 |
![]() |
![]() |
−1.5 ± 0.21 | 6.9 |
16 | XRT 150322/ | 16453 | 74.7 | 2015-03-21/22 | 10.3![]() |
53.07672 | –27.87345 |
![]() |
![]() |
−0.33 ± 0.08 | 35.2 |
CDF-S XT2 ( † ) | |||||||||||
17 | XRT 151121 | 18715 | 24.5 | 2015-11-20/21 | 5.5![]() |
40.82972 | 32.32390 |
![]() |
![]() |
−0.17 ± 0.20 | 6.4 |
18 | XRT 161125 | 19310 | 6.1 | 2016-11-25 | 2.9![]() |
36.71489 | –1.08317 |
![]() |
![]() |
−0.64 ± 0.18 | 4.3 |
19 | XRT 170901 ( † ) | 20635 | 77.0 | 2017-08-31/09-01 | 3.9![]() |
356.26437 | –42.64494 |
![]() |
![]() |
+0.00 ± 0.08 | 43.7 |
20 | XRT 191127 | 21831 | 22.5 | 2019-11-26/27 | 0.3±0.2 | 207.34711 | 26.58421 |
![]() |
![]() |
−0.34 ± 0.17 | 8.6 |
21 | XRT 191223 | 23103 | 18.1 | 2019-12-23 | 3.7![]() |
50.47516 | 41.24704 |
![]() |
![]() |
−0.16 ± 0.20 | 9.7 |
22 | XRT 210423 ( † ) | 24604 | 26.4 | 2021-04-23/24 | 12.1![]() |
207.23523 | 26.66230 |
![]() |
0![]() |
−0.18 ± 0.10 | 12.4 |
Notes. Column 1: shorthand identifier (FXT #) used throughout this work. Column 2: X-ray transient identifier (XRT date), plus previous name when available. Columns 3–5: Chandra observation ID, exposure time in units of ks, and date. Column 6: T90 duration, which measures the time over which the source emits the central 90% (i.e., from 5% to 95%) of its total measured counts, in units of ks. Columns 7 and 8: Right Ascension and Declination in J2000 equatorial coordinates. Column 9: off-axis angle of the FXT candidates, with respect to the Chandra aimpoint, in units of arcminutes. Column 10: estimated 2σ X-ray positional uncertainty, in units of arcseconds (see Sect. 2.5). Column 11: hardness ratio (HR) and 1σ uncertainty, defined as HR = (H − S)/(H + S) where H = 2 − 7 keV and S = 0.5 − 2 keV energy bands, using the Bayesian estimation of Park et al. (2006). Column 12: approximate signal-to-noise ratio (S/N). ( † )Previously reported as FXTs by Xue et al. (2019) for FXT 16, Lin et al. (2019) for FXT 19, and Lin et al. (2021) in the case of FXT 22.
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