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Table 2.

Physical and X-ray properties of very red giant stars identified with X-ray sources.

Gaia DR3 ID Name BP-RP Gabs Spec CR Err Exp. Li fX, −14 log(LX) FUV – NUV
4644856055150677632 CI Hyi 4.31 −2.27 M5/7III 0.083 0.023 217.6 26.8 7.50 30.69 n.a.
4748477123328077696 R Hor 5.60 −0.70 M5-7e 1.143 0.072 224.4 1447.2 102.86 ( * ) 31.38 ( * ) n.a.
5159194331764625920 DR Eri 2.64 −1.96 M2/3III 0.030 0.014 191.0 7.8 2.66 30.31 0.29
5100253911446411264 BH Eri 3.86 −2.34 M6 0.082 0.023 195.2 27.5 7.40 30.98 n.a.
4723045075781077760 UU Ret 2.64 −2.31 M3III 0.023 0.009 400.2 13.4 2.10 30.43 n.a.
4616109220563904768 U Men 3.75 0.53 M3e 0.647 0.052 266.4 637.2 58.24 ( * ) 31.28 ( * ) 2.35
4772353701224784640 CD-51 1503 2.96 −1.90 S5,2 0.113 0.017 451.0 105.3 10.19 31.08 n.a.
4620697620025724544 CPD-8486 3.01 −1.64 S4,4 0.071 0.017 314.5 41.6 6.43 30.71 2.59
893132234387415808 BD+32 1528 3.08 −1.12 0.068 0.032 77.0 11.0 6.14 30.87 1.91
5193680960648176768 TYC9506-1836-1 3.79 −1.52 0.063 0.015 357.2 41.7 5.63 30.76 3.13
5761301055347596800 MV Hya 2.63 −1.95 M3/4III 0.050 0.026 87.8 9.2 4.50 30.38 n.a.
645414291872801536 EH Leo 2.76 −2.84 0.296 0.066 75.2 71.1 26.68 31.31 2.09
5195956296883496832 HD 84048 2.58 −1.84 M1/2 0.067 0.014 396.9 56.1 6.04 30.80 0.41
794754943320201600 R LMi 6.31 −0.33 M6.5-9e 0.079 0.033 79.7 18.0 7.15 ( * ) 30.32 ( * ) n.a.
3491583497096278144 WW Crt 2.85 −1.18 M4III 0.653 0.076 128.1 287.9 58.78 31.25 3.35
6173329362681684736 TW Cen 5.30 −1.34 M6-8Ib-II 0.067 0.022 172.0 18.5 6.06 30.67 3.99
6738529604088911104 IRAS19204-3959 3.16 −0.70 0.061 0.032 82.2 8.9 5.52 30.82 n.a.
6713213967334901376 HD 181817 2.51 −2.04 M2III 0.061 0.029 83.7 10.3 5.47 30.65 2.68
6342796540114659200 HD 199203 2.56 −2.55 M2/3(III) 0.076 0.024 177.4 20.9 6.86 30.86 n.a.

Notes. Columns 1 and 2 give the Gaia DR3 IDs and another name of the sources. Columns 3 and 4 give the HR diagram position (i.e., the Gaia BP-RP color and absolute G magnitude). Column 5 provides a spectral type estimate. Columns 6 and 7 list the recorded count rates per second and the corresponding errors. Column 8 reports the exposure time in seconds, and column 9 shows the detection likelihood. Column 10 provides the X-ray flux in 10−14 erg s−1. Column 11 gives the derived X-ray luminosities in erg s−1, and column 12 gives the FUV-NUV colors derived from GALEX. (See text for details.) The stars marked with “*” are likely affected by optical contamination (again, see text for details).

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