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Table 2.

LS10 counterparts of TDE candidates with their probabilities (p_any) and redshifts (z).

Name p_any LS10_RA LS10_Dec z
[deg] [deg]
1 J0114 0.43 18.6286 −59.6152 0.16
2 J0141 0.38 25.3891 −44.5707 0.09
3 J0240 0.99 40.2062 −59.9091 0 . 21 − 0.04 + 0.07 $ 0.21^{+0.07}_{-0.04} $
4 J0318 0.32 49.7388 −20.9143 0 . 27 − 0.09 + 0.13 $ 0.27^{+0.13}_{-0.09} $
5 J0340 0.99 55.0208 −38.0005 0 . 21 − 0.05 + 0.06 $ 0.21^{+0.06}_{-0.05} $
6 J0341 0.99 55.3219 −45.9553 0 . 34 − 0.11 + 0.08 $ 0.34^{+0.08}_{-0.11} $
7 J0439 0.98 69.9986 −65.2342 0.15
8 J0608 0.77 92.1226 −43.8892 0.08
9 J0615 0.92 93.7837 −44.9893 0 . 10 − 0.03 + 0.03 $ 0.10^{+0.03}_{-0.03} $
10 J0634 0.70 98.5558 −71.6518 0.13
11 J0644 0.58 101.2052 −60.6178 0.12
12 J0707 0.24 106.7895 −84.346 0 . 17 − 0.02 + 0.23 $ 0.17^{+0.23}_{-0.02} $
13 J0744 – 116.1089 29.2688 0.04
14 J0820 0.95 125.2324 19.427 0.12
15 J0823 0.99 125.9032 4.384 0.03
16 J0847 0.99 131.8265 −75.1814 –
17 J0916 0.16 139.2407 6.1658 0.09
18 J1102 0.26 165.6673 −5.3031 0 . 33 − 0.09 + 0.10 $ 0.33^{+0.10}_{-0.09} $
19 J1305 0.06 196.3994 1.7837 0 . 33 − 0.08 + 0.07 $ 0.33^{+0.07}_{-0.08} $
20 J1401 0.96 210.492 8.2337 0 . 26 − 0.05 + 0.06 $ 0.26^{+0.06}_{-0.05} $
21 J1421 0.12 215.4155 −29.8896 0.06
22 J1436 0.85 219.0989 −17.6845 0 . 19 − 0.03 + 0.06 $ 0.19^{+0.06}_{-0.03} $
23 J1456 0.95 224.0958 −28.6487 0.09
24 J1459 0.02 224.978 −26.1409 0.09
25 J1534 0.99 233.5261 −9.0593 0.02
26 J1646 0.21 251.7032 −69.4271 0.02
27 J1730 0.88 262.6191 −85.0844 0 . 33 − 0.05 + 0.07 $ 0.33^{+0.07}_{-0.05} $
28 J1901 0.9 285.4461 −55.3662 0.06
29 J1921 0.97 290.3667 −50.4652 0.06
30 J2108 0.98 317.2424 −56.4753 0.04
31 J2344 0.49 356.0123 −35.4449 0.10

Notes. Photometric redshifts are noted with their 1σ errors, others are spectroscopic. The origin of redshifts as well as more counterpart properties can be found in the eRO-ExTra catalog. The photo-z for J0847 is not-reliable, since two optical photometry griz points were missing in the calculation; it is therefore not listed. The p_any value for J0744 is omitted, since the counterpart was identified in Malyali et al. (2023a).

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