Table 4
Extended sources in field, MCMF associations, and derived quantities.
| ID | Name | α | δ | zphot | fcont | kBT | fx | LX | M500,LX | M500,kT |
|---|---|---|---|---|---|---|---|---|---|---|
| X1 | SRGEJ043217.5-610359 | 68.0729 | −61.0666 | 0.364 | 0.00 |  |
−13.17 ± 0.01 | 43 49 ± 0 01 | 14.2 ± 0.1 | 14.3 ± 0.2 |
| X2 | SRGE J043324.0-610801 | 68.3498 | −61.1336 | 0.745 | 0.00 |  |
−13.41 ± 0.02 |  |
14.4 ± 0.1 | 14.5 ± 0.2 |
| X3 | SRGEJ043208.6-615106 | 68.0358 | −61.8518 | 1.05 | 0.07 |  |
−13.44 ± 0.02 |  |
14.5 ± 0.1 | 14.5 ± 0.3 |
| X4 | SRGE J043317.2-614035 | 68.3217 | −61.6765 | 0.532 | 0.00 |  |
−13.58 ± 0.03 |  |
14.2 ± 0.1 | 14.4 ± 0.3 |
| X5 | SRGE J043327.9-612722 | 68.3664 | −61.4563 | 0.717 | 0.00 |  |
−13.73 ± 0.03 |  |
14.2 ± 0.1 | 14.5 ± 0.3 |
| X6 | SRGE J043224.4-614519 | 68.1016 | −61.7553 | 0.907 | 0.06 |  |
−13.75 ± 0.03 |  |
14.3 ± 0.1 | 14.4 ± 0.3 |
| X7 | SRGE J042900.3-610243 | 67.2512 | −61.0455 | 0.0458 | 0.35 |  |
 |
 |
13.0 ± 0.1 | – |
| X8 | SRGE J042943.9-611038 | 67.4330 | −61.1773 | 0.0487 | 0.14 |  |
 |
 |
13.3 ± 0.1 | 13.7 ± 0.2 |
| X9 | SRGEJ042746.8-611858 | 66.9451 | −61.3162 | 0.457 | 0.28 |  |
 |
 |
14.0 ± 0 1 | 14.3 ± 0.3 |
| X10 | SRGEJ042734.6-611613 | 66.8941 | −61.2705 | 0.338 | 0.53 |  |
 |
 |
13.7 ± 0 1 | – |
| X11 | SRGE J043432.5-612153 | 68.6353 | −61.3649 | 0.672 | 0.03 |  |
 |
 |
13.9 ± 0 2 | – |
Notes. Shown is the short ID used in this paper, the SRG source name, the J2000 position of the source in decimal degrees (α, δ), the photometric redshift of the most likely MCMF identification (zphot), the MCMF probability of contamination of the most likely identification (fcont), the best fitting X-ray temperature (kBT;keV), the 0.5–2.0 keV X-ray flux (fX; log10 erg cm−2 s−1), the 0.5–2.0 keV rest X-ray luminosity (LX; log10 erg s−1), and M500 cluster masses assuming luminosity-mass (M500,LX; log10 M⊙) and temperature-mass (M500,kT; log10 M⊙) scaling relations. X8 was fitted by a two apec components, of which we only show the properties of the coolest one here.
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