Table A.1.
Sources per FXT for which we extracted spectra from the MUSE cubes, according to the selection criteria explained in Section 3.2.
| Source | RA | Dec | mR, AB | Lines detected | z | DL | offset | LX, peak | MR, AB | Pch |
|---|---|---|---|---|---|---|---|---|---|---|
| (degrees) | (degrees) | (Gpc) | (kpc) | (1044 erg s−1) | ||||||
| XRT 030510 | ||||||||||
| 2 | 76.78438 | -31.8761 | 22.54±0.05 | [OII], Hβ, [OIII] | 0.65510(1) | 4.0 | 216±4 | 45 | -20.49±0.05 | 0.9846 |
| 4 | 76.78093 | -31.875 | 24.91±0.15 | [OII], [OIII] | 0.628611(6) | 3.8 | 149±4 | 40 | -18.01±0.15 | 1.0 |
| 5 | 76.7816 | -31.87499 | 25.11±0.17 | [OII], Hβ, [OIII] | 0.73252(6) | 4.6 | 165±4 | 59 | -18.22±0.17 | 1.0 |
| 12 | 76.77125 | -31.87208 | 21.7±0.03 | [OII], Hβ, [OIII]λ5007Å, Ca H+K | 0.48551(3) | 2.8 | 141±3 | 21 | -20.54±0.03 | 0.7111 |
| 14 | 76.77442 | -31.87156 | 23.8±0.09 | [OIII] | 0.54879(2) | 3.3 | 87±3 | 29 | -18.77±0.09 | 0.8783 |
| 19 | 76.78326 | -31.87029 | 24.63±0.13 | [OII], [OIII], Hα | 0.30944(3) | 1.7 | 75±2 | 7 | -16.47±0.13 | 0.9969 |
| 20 | 76.77127 | -31.87026 | 21.1±0.03 | [OII], Hβ, [OIII] | 0.62900(4) | 3.8 | 148±4 | 40 | -21.83±0.03 | 0.4858 |
| 22 | 76.77946 | -31.86843 | 22.52±0.05 | [OII], Hβ, [OIII] | 0.46611(3) | 2.7 | 36±3 | 19 | -19.62±0.05 | 0.1466 |
| 23 | 76.77897 | -31.86818 | 22.580.05 | [OII], Hβ, [OIII] | 0.4370(1) | 2.5 | 343 | 17 | -19.40.05 | 0.1461 |
| 25 | 76.7752 | -31.86799 | 23.36±0.07 | [OII] | 1.357 | 9.9 | 92±5 | 269 | -21.62±0.07 | 0.6186 |
| 27 | 76.7713 | -31.86718 | 24.82±0.15 | Hβ, [OIII] | 0.68966(3) | 4.3 | 165±4 | 51 | -18.35±0.15 | 1.0 |
| 32 | 76.76918 | -31.86638 | 23.28±0.07 | [OII] | 0.997 | 6.8 | 244±4 | 125 | -20.87±0.07 | 0.9992 |
| 37 | 76.76946 | -31.86383 | 23.50.08 | [OII], [OIII] | 0.30729(9) | 1.6 | 1572 | 7 | -17.580.08 | 1.0 |
| 43 | 76.77866 | -31.86172 | 26.290.29 | [OII], Hβ, [OIII] | 0.5047(1) | 2.9 | 1803 | 23 | -16.060.29 | 1.0 |
| 44 | 76.77353 | -31.86169 | 23.86±0.09 | [OII] | 1.1 | 7.6 | 267±4 | 160 | -20.55±0.09 | 1.0 |
| XRT 100831 | ||||||||||
| 2 | 90.0105 | -52.72306 | 23.79±0.09 | [OII], Hβ, [OIII] | 0.56071(6) | 3.3 | 214±6 | 11 | -18.83±0.09 | 1.0 |
| 6 | 90.00257 | -52.72208 | 25.26±0.18 | [OII], Hβ, [OIII] | 0.72433(3) | 4.6 | 193±6 | 22 | -18.04±0.18 | 1.0 |
| 8 | 90.015 | -52.72125 | 21.17±0.03 | [OII], Hβ, [OIII], Ca H+K | 0.55973(9) | 3.3 | 215±6 | 11 | -21.45±0.03 | 0.81 |
| 9 | 90.0104 | -52.72072 | 21.7±0.03 | [OII], Hβ, [OIII], Hα, Ca H+K | 0.27709(6) | 1.5 | 107±4 | 2 | -19.13±0.03 | 0.7624 |
| 19 | 90.01407 | -52.71556 | 25.90.24 | [OII] | 1.100 | 7.6 | 1787 | 62 | -18.520.24 | 1.0 |
| 21† | 90.00428 | -52.71513 | 26.470.31 | [OII] | 1.22 | 8.7 | 67 | 80 | -18.220.31 | 0.0435 |
| 24 | 89.99377 | -52.71502 | 24.27±0.11 | [OII] | 1.011 | 6.9 | 191±7 | 50 | -19.92±0.11 | 0.9999 |
| 25 | 90.00977 | -52.71465 | 24.98±0.16 | [OII], Hβ, [OIII]λ5007Å | 0.61107(2) | 3.7 | 82±6 | 14 | -17.87±0.16 | 0.9834 |
| 26 | 89.99254 | -52.71467 | 26.24±0.28 | [OII] | 1.009 | 6.9 | 214±7 | 50 | -17.94±0.28 | 1.0 |
| 31 | 90.01075 | -52.71374 | 23.61±0.08 | Hβ, [OIII], Hα | 0.2265(8) | 1.2 | 54±3 | 1 | -16.71±0.08 | 0.8881 |
| 36 | 90.00258 | -52.71291 | 23.23±0.07 | [OII], Hβ, [OIII] | 0.6031(2) | 3.7 | 58±6 | 14 | -19.58±0.07 | 0.4209 |
| 38 | 90.01374 | -52.71222 | 24.41±0.12 | [OII] | 0.610 | 3.7 | 157±6 | 14 | -18.44±0.12 | 0.9999 |
| 39 | 90.01687 | -52.71237 | 22.61±0.05 | Hβ, [OIII]λ5007Å, Hα | 0.14225(2) | 0.7 | 74±2 | 0 | -16.6±0.05 | 0.981 |
| 41 | 89.9922 | -52.71152 | 25.36±0.19 | [OII] | 1.385 | 10.2 | 254±7 | 109 | -19.68±0.19 | 1.0 |
| 48 | 89.99782 | -52.70943 | 20.63±0.02 | [OII], Hβ, [OIII], Hα | 0.323714(5) | 1.7 | 119±4 | 3 | -20.58±0.02 | 0.4692 |
| 49 | 90.00501 | -52.70799 | 23.31±0.07 | [OII], Hβ, [OIII], Hα | 0.32371(4) | 1.7 | 121±4 | 3 | -17.9±0.07 | 0.9946 |
| XRT 060207 | ||||||||||
| 2 | 196.83312 | -40.46675 | 25.05±0.16 | [OII] | 0.795 | 5.1 | 163±15 | 82 | -18.5±0.16 | 1.0 |
| 4 | 196.82867 | -40.46728 | 20.23±0.02 | Ca H+K | 0.58811(4) | 3.5 | 170±13 | 39 | -22.52±0.02 | 0.3802 |
| 10 | 196.82279 | -40.46511 | 24.29±0.11 | [OII] | 1.429 | 10.5 | 259±16 | 349 | -20.82±0.11 | 1.0 |
| 11 | 196.83542 | -40.46528 | 23.24±0.07 | [OII], Hβ, [OIII] | 0.44222(4) | 2.5 | 106±11 | 19 | -18.76±0.07 | 0.9212 |
| 12 | 196.82467 | -40.46517 | 22.00±0.04 | [OII], Hβ, [OIII], Ca H+K | 0.53148(4) | 3.1 | 167±12 | 31 | -20.48±0.04 | 0.863 |
| 15 | 196.82317 | -40.46425 | 22.82±0.06 | [OII], Hβ, [OIII] | 0.72830(7) | 4.6 | 205±14 | 66 | -20.49±0.06 | 0.9864 |
| 20 | 196.84221 | -40.46281 | 24.21±0.11 | [OII] | 0.884 | 5.8 | 226±15 | 106 | -19.62±0.11 | 1.0 |
| 25 | 196.84233 | -40.46228 | 23.76±0.09 | [OII], Hβ, [OIII] | 0.59278(2) | 3.6 | 193±13 | 40 | -19.01±0.09 | 0.9999 |
| 36 | 196.83279 | -40.46094 | 24.51±0.13 | [OII] | 0.939 | 6.3 | 14±15 | 123 | -19.48±0.13 | 0.0575 |
| 37 | 196.8215 | -40.46081 | 24.66±0.14 | [OII] | 1.153 | 8.1 | 248±16 | 205 | -19.88±0.14 | 1.0 |
| 41 | 196.84154 | -40.45983 | 21.1±0.03 | [OII], Ca H+K | 0.591164(1) | 3.6 | 177±13 | 40 | -21.67±0.03 | 0.6364 |
| 42 | 196.83575 | -40.45864 | 24.31±0.12 | [OII] | 1.157 | 8.1 | 108±16 | 207 | -20.24±0.12 | 0.9454 |
| 43 | 196.82512 | -40.458 | 23.83±0.09 | [OII] | 1.385330(1) | 10.2 | 190±16 | 323 | -21.2±0.09 | 0.9974 |
| 44 | 196.83625 | -40.45797 | 20.24±0.02 | [OII] | 0.986 | 6.7 | 126±16 | 139 | -23.88±0.02 | 0.1682 |
| 45 | 196.8275 | -40.45833 | 22.0±0.04 | Ca H+K | 0.58761(7) | 3.5 | 108±13 | 39 | -20.75±0.04 | 0.5268 |
| 46 | 196.82804 | -40.45772 | 21.72±0.04 | [OII] | 0.767 | 4.9 | 123±14 | 75 | -21.73±0.04 | 0.4674 |
| 48 | 196.82937 | -40.45728 | 21.92±0.04 | [OII], Hβ, [OIII] | 0.62575(8) | 3.8 | 107±13 | 45 | -21.0±0.04 | 0.4786 |
| 51 | 196.82308 | -40.45669 | 22.03±0.04 | [OII], Hβ, [OIII] | 0.58731(4) | 3.5 | 199±13 | 39 | -20.72±0.04 | 0.9268 |
| 55 | 196.8275 | -40.45606 | 21.38±0.03 | Ca H+K | 0.58839(6) | 3.5 | 148±13 | 39 | -21.36±0.03 | 0.5848 |
| 57 | 196.83033 | -40.45503 | 24.68±0.14 | Hβ, [OIII]λ5007Å | 0.624(2) | 3.8 | 152±13 | 45 | -18.23±0.14 | 1.0 |
| 59 | 196.828 | -40.45511 | 22.25±0.04 | Ca H+K | 0.73265(8) | 4.6 | 178±14 | 67 | -21.08±0.04 | 0.873 |
| 63 | 196.83371 | -40.45233 | 23.72±0.09 | [OII] | 1.430 | 10.6 | 270±16 | 350 | -21.4±0.09 | 1.0 |
| XRT 070618 | ||||||||||
| 0 | 24.27846 | -12.96053 | 22.96±0.06 | [OII], Hβ, [OIII] | 0.431 | 2.4 | 179±5 | 75 | -18.99±0.06 | 0.9975 |
| 2 | 24.27712 | -12.96017 | 22.34±0.05 | [OII] | 1.291 | 9.3 | 243±8 | 1087 | -22.51±0.05 | 0.9554 |
| 3 | 24.27712 | -12.95964 | 22.32±0.05 | [OII], Hβ, [OIII], Hα | 0.36744(2) | 2.0 | 138±5 | 51 | -19.22±0.05 | 0.9304 |
| 6 | 24.27108 | -12.95933 | 24.87±0.15 | [OII], Hβ, [OIII], Hα | 0.36758(1) | 2.0 | 150±5 | 51 | -16.67±0.15 | 1.0 |
| 9 | 24.27462 | -12.95764 | 24.73±0.14 | [OII] | 1.223 | 8.7 | 158±8 | 951 | -19.97±0.14 | 0.9998 |
| 14 | 24.27587 | -12.95586 | 21.16±0.03 | [OII], Hβ, [OIII], Ca H+K | 0.43200(1) | 2.5 | 71±5 | 75 | -20.78±0.03 | 0.209 |
| 17 | 24.27162 | -12.95489 | 23.25±0.07 | [OII], Hβ, [OIII] | 0.44380(3) | 2.5 | 90±5 | 80 | -18.76±0.07 | 0.8431 |
| 22 | 24.28117 | -12.95281 | 18.86±0.01 | Ca H+K | 0.2080(1) | 1.1 | 72±3 | 14 | -21.26±0.01 | 0.108 |
| 23 | 24.282 | -12.95108 | 21.01±0.03 | [OII], Ca H+K | 0.660367(1) | 4.1 | 174±6 | 209 | -22.04±0.03 | 0.5629 |
| 26 | 24.27038 | -12.95019 | 23.19±0.07 | [OII] | 0.921 | 6.1 | 154±7 | 472 | -20.75±0.07 | 0.9369 |
| 27 | 24.27629 | -12.95014 | 22.86±0.06 | [OII], [OIII] | 0.60702(3) | 3.7 | 65±6 | 170 | -19.97±0.06 | 0.4039 |
| 30 | 24.27279 | -12.94792 | 22.99±0.06 | [OII], [OIII]λ5007Å, Hα | 0.36762(2) | 2.0 | 99±5 | 51 | -18.54±0.06 | 0.898 |
| 33 | 24.27587 | -12.94758 | 21.29±0.03 | [OII], Hβ, [OIII], Ca H+K | 0.48739(2) | 2.8 | 112±6 | 100 | -20.97±0.03 | 0.4302 |
Notes. †See Section 5.2 for how this redshift was obtained. The source numbers are indicated in Figure 1. RA and Dec are the source’s centroid coordinates in the R-band images and the apparent magnitude is the Kron magnitude in the R-band images, uncorrected for Galactic extinction. We also indicate what emission and/or absorption lines were identified in the spectra to obtain the redshift. The redshift is presented with the estimated uncertainty in the last digit between brackets. The distance is the luminosity distance calculated using the DISTANCE module within ASTROPY.COSMOLOGY using the redshift listed in the table. The offset is calculated between the centroid positions of the FXT and the candidate host galaxy, using only the error on the FXT position to calculate the error on the offset. LX, peak is reported in the 0.3–10 keV energy range. The absolute magnitude (uncorrected for Galactic extinction) is calculated using the distance listed in the table and Pch is calculated as described in Section 3.6.
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