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Table 8

Observed X-ray flux (0.2–2.3 keV) and intrinsic luminosity (0.3–10.0 keV) of eRASS1 X-AGBs.

IRAS number Common name fX (10−14 erg cm−2 s−1) Distance (pc) LX (1030 erg s−1) L/L (×103) LX/L (×10−6) log(LX/L) TX (MK)
High confidence X-AGB stars
02346–6248 RS Hor 6.4 ± 3.0 1710 ± 160 64 ± 32 1.7 9.8 −5.0
05166–2215 RZ Lep 10.6 ± 4.2 1070 ± 60 41 ± 17 1.8 6.0 −5.2
06024–8403 CPD–8486 5.8 ± 1 .5 793 ± 20 8.3 ± 1 .6 1.2 1.7 −5.8 30 ± 23
12118–5115 TV Cen 7.3 ± 3.2 849±17 18±8 0.59 7.9 −5.1
13548–3049 TWCen 15±5 770 ± 70 30 ± 12 3.7 2.1 −5.7
14188–6943 VXCir 13±5 2450 ± 430 115 ± 60 25.4 1.2 −5.9 175+78$17_{ - 5}^{ + 78}$
16263–4910 20 ± 10 1550 ± 260 160 ± 100 1.6 26.9 −4.6 22 ± 8
Possible X-AGB stars
11390–7213 MQMus 5.3 ± 1.8 2040 ± 360 75 ± 37 7.3 2.7 −5.6
11510–6046 V1245 Cen 7.1 ± 2.9
CGCS 3366 10.8 ± 4.0 5000 ± 700 910 ± 420 0.8 290 −3.5
13494–0313 HD 120832 18 ± 6 853 ± 34 45 ± 15 0.7 17 −4.8
16047–5449 V501 Nor 9.3 ± 4.2 2020 ±190 130 ± 60 7.2 4.7 −5.3
17023–5859 CH Ara 8.6 ± 4.4 3700 ±1000 390 ± 290 7.8 13 −4.9
V371 CrA 17±8

Notes. As described in the text, the relative uncertainty in L/L is smaller to 42%+74%$ \approx _{ - 42{\rm{\% }}}^{ + 74{\rm{\% }}}$.

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