Table 2
Results of source detection and ML PSF fitting.
| Parameter | |
|---|---|
| # X-ray sources (FoV) | |
| … 0.2–0.6 keV | 508 |
| … 0.6–2.3 keV | 968 |
| … 2.3–5.0 keV | 279 |
| Detection likelihood | 5 × 106 |
| ML Counts | |
| … 0.2–0.5 keV | 5.7258(9) × 105 |
| … 0.5–1.0 keV | 2.220(3) × 105 |
| … 1.0–2.2 keV | 1.690(13) × 104 |
| … 2.2–10 keV | 4.41(25) × 102 |
| Rate (s−1) | 7.697(9) |
| (†)HR1 | −0.4412(6) |
| (†)HR2 | −0.8585(10) |
| (†)HR3 | −0.9492(28) |
| RA (h min s) | 6:59:48.3 |
| Dec (d m s) | 14:14:20.993 |
Notes. Detection likelihood, count rate, and equatorial coordinates as computed with the task ermldet in the total eROSITA energy band, considering all active telescope modules (except for TM1) and all valid patterns.(†) Hardness ratios are the ratios of the difference to total counts in two contiguous of four eROSITA energy bands: 0.2–0.5 keV, 0.5–1 keV, 1–2.2 keV, and 2.2–10 keV.
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