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Table 2.

Properties of the selected candidates.

Source RA Dec Error (a) b Pno-match(b) Separation (c) HR1 (d) HR2 (d) HR3 (d) CTS (e) Texp(f) Magnitude (g) Filter (h) fX/fopt(i)
eRASSU [°] [°] [″] [°] [%] [″] [s] limit [mag]
J052152.0−503812 80.467 −50.6369 1.16 −34.58 100 5.81″(5.01σ) 0.44(0.08) −0.37(0.08) −0.96(0.07) 232 3226 25.48 r 449
J062748.5−260240 96.9523 −26.0446 1.50 −16.41 60 2.99″(2.00σ) 0.3(0.14) −0.52(0.15) −1.0(0.15) 64 964 21.73 r 14
J065715.3+260428 (j) 104.314 26.0746 1.31 12.75 100 15.15″(11.6σ) 0.33(0.11) −0.79(0.09) −1.0(0.26) 88 659 22.21 r 859
J071828.7+141044 109.62 14.1789 2.05 12.31 84 5.32″(2.59σ) 1.0(0.4) 0.55(0.17) −1.0(0.05) 27 630 22.16 r 118
J072302.3−194225 110.7599 −19.7071 1.62 −2.21 83 5.50″(3.40σ) −0.22(0.15) −0.98(0.12) 0.7(1.3) 53 764 21.93 r 22
J072635.8−001642 111.6496 −0.2785 2.52 7.69 91 6.24″(2.48σ) 0.85(0.26) 0.47(0.17) −1.0(0.13) 36 652 21.92 r 24
J080701.3+023823 121.7558 2.6398 1.76 17.99 54 6.17″(3.51σ) 0.52(0.16) −0.23(0.17) −0.85(0.28) 47 598 24.50 r 512
J080717.2−182019 121.8217 −18.3387 1.95 7.53 52 2.90″(1.49σ) 0.6(0.15) −0.56(0.15) −1.0(0.15) 47 697 22.00 r 17
J081952.1−131930 124.9672 −13.3251 1.38 12.76 100 8.56″(6.21σ) −0.88(0.07) −1.0(0.23) 1.0(5.0) 78 677 22.99 r 146
J083039.8+353102 127.6661 35.5172 1.96 34.67 100 7.79″(3.98σ) 0.56(0.24) 0.14(0.22) −1.0(0.12) 29 574 24.12 r 263
J084046.2−115222 130.1926 −11.873 1.65 17.82 79 7.18″(4.34σ) −0.39(0.13) −1.0(0.09) 1.0(2.7) 51 622 22.12 r 36
J085257.5+270013 133.2399 27.0039 1.92 37.45 100 9.45″(4.91σ) 0.58(0.19) −0.14(0.18) −0.95(0.11) 40 577 24.56 r 425
J085351.2+272536 133.4634 27.4268 2.42 37.75 86 7.57″(3.13σ) 1.0(0.4) 0.72(0.14) −0.73(0.14) 32 585 24.51 r 1217
J090421.1−383956 136.0882 −38.6656 1.60 5.50 100 7.09″(4.44σ) 1.0(0.04) −0.42(0.13) −1.0(0.13) 63 919 23.64 r 67
J093317.6−251252 143.3236 −25.2147 1.28 19.17 62 3.99″(3.13σ) 0.42(0.13) −0.22(0.13) −0.84(0.13) 94 695 22.35 r 75
J100957.4+125914 152.4893 12.9873 2.92 49.75 50 6.71″(2.30σ) 0.43(0.21) −0.43(0.21) −0.7(0.4) 29 525 24.62 r 154
J101110.9+083329 152.7957 8.5582 1.86 47.85 58 6.43″(3.45σ) 0.42(0.21) −0.16(0.2) −1.0(0.1) 36 542 24.63 r 223
J103951.1+323442 159.9631 32.5785 2.35 61.07 100 11.40″(4.86σ) 0.35(0.25) 0.04(0.23) −0.8(0.23) 27 609 24.35 r 338
J110240.2−250706 165.6678 −25.1184 1.33 31.55 99 5.17″(3.88σ) 0.35(0.11) −0.47(0.12) −0.78(0.2) 104 815 24.65 r 606
J113351.2−522712 173.4634 −52.4535 1.18 8.63 80 2.96″(2.51σ) 0.55(0.1) −0.75(0.09) −0.8(0.4) 99 1672 23.37 r 55
J121826.7+071144 184.6113 7.1956 2.28 68.59 56 4.52″(1.98σ) 0.38(0.24) 0.0(0.2) −0.89(0.16) 35 715 24.69 r 170
J122150.6−193438 185.4611 −19.5774 1.40 42.75 99 5.31″(3.79σ) 0.6(0.12) −0.38(0.12) −0.9(0.13) 85 1083 24.48 r 207
J125214.5−591759 193.0606 −59.2999 1.04 3.57 85 0.59″(0.57σ) 0.47(0.08) −0.84(0.06) −0.7(0.4) 164 1802 23.32 r 77
J130406.1−533816 196.0256 −53.6379 1.13 9.19 99 3.75″(3.32σ) 0.44(0.08) −0.86(0.06) −0.7(0.4) 147 1735 23.24 r 63
J130821.3+130319 197.0891 13.0555 1.69 75.38 100 7.42″(4.39σ) 0.58(0.15) −0.13(0.15) −1.0(0.13) 75 1060 24.63 r 206
J131716.9−402647 (j) 199.3205 −40.4464 0.83 22.16 100 5.16″(6.21σ) 0.42(0.07) −0.85(0.04) −1.0(0.28) 415 1464 24.88 r 10 801
J133355.8−665647 203.4828 −66.9466 0.81 −4.42 65 1.64″(2.03σ) 0.79(0.04) −0.73(0.04) −1.0(0.026) 468 1836 23.31 r 188
J134725.4−363415 206.8561 −36.5709 1.31 24.95 99 4.50″(3.42σ) −0.26(0.12) −1.0(0.1) 100 1376 25.00 r 381
J174858.8−510951 267.245 −51.1642 0.92 −11.83 100 5.60″(6.10σ) 0.19(0.07) −0.84(0.05) −1.0(0.12) 256 920 21.21 g 31
J175415.0−740127 268.5625 −74.0244 1.58 −22.20 84 4.43″(2.81σ) 0.41(0.15) −0.27(0.15) −0.83(0.19) 66 1198 24.84 r 194
J175532.5−503748 268.8858 −50.6301 1.47 −12.48 77 4.89″(3.33σ) 0.72(0.09) −0.87(0.07) −1.0(0.5) 82 846 21.33 g 11
J183349.6−353707 278.4569 −35.6188 2.18 −12.12 56 4.49″(2.06σ) 0.55(0.2) −0.13(0.19) −0.92(0.19) 42 666 20.89 g 17
J214920.9−443050 327.3374 −44.514 1.77 −49.85 53 4.29″(2.42σ) 0.7(0.21) 0.09(0.19) −0.79(0.15) 38 673 25.24 r 298

Notes. During the observations, eROSITA was operated in SURVEY mode.

(a)

1σ positional accuracy. Calculated as described in Table 2 of Kurpas et al. (2023).

(b)

Probability from the ARCHES cross-match that the eROSITA source has no counterpart in any of the wide area optical or IR catalogues.

(c)

Angular distance to the closest optical or IR source.

(d)

Hardness ratio values. HR1 is computed between the 0.2–0.5 keV and 0.5–1 keV bands, HR2 between the 0.5–1 keV and 1–2 keV bands, and HR3 between the 1–2 keV and 2–5 keV bands.

(e)

Number of detected counts in the 0.2–2 keV band.

(f)

Total CCD live time, uncorrected for vignetting effects.

(g)

Local magnitude limit computed from neighboring optical sources.

(h)

Passband of the local magnitude limit. The term r refers to the Pan-STARRS, Legacy Survey, or DeCAPS2 r-band, whereas g marks magnitudes in the Gaia g-band. All magnitudes are given in the AB system.

(i)

The X-ray-to-optical flux ratio, in relation to the V-band, was computed via log ( f X / f opt ) = log ( F X erg s 1 c m 2 ) + m 2.5 + 5.39 $ \log(f_{\mathrm{X}}/f_{\mathrm{opt}}) = \log(\frac{F_{\mathrm{X}}}{\mathrm{erg\,s}^{-1}\,cm^{-2}}) +\frac{m}{2.5}+5.39 $, with FX as the X-ray flux and m the local magnitude limit. See Sect. 3.4 for more details.

(j)

We list the derived properties for J06571 and J13171 also in this table, although they were already published in Kurpas et al. (2023) and Kurpas et al. (2024).

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