Table 1.
X-ray and space-based optical/UV observations of J0428−00.
| Instrument | ObsID | Date (MJD) | X-ray Exp. (in ks) | Optical & UV filters (exp. in ks) |
|---|---|---|---|---|
| Swift | 00013199001 | 58886 | 2.0 | V(0.17), B(0.17), U(0.17), W1(0.3), M2(0.37), W2(0.67) |
| Swift | 00013199003 | 58895 | 1.4 | V(0.1), B(0.1), U(0.1), W1(0.20), M2(0.35), W2(0.44) |
| Swift | 00013199004 | 58899 | 0.7 | B(0.09), U(0.09), W1(0.26), W2(0.2) |
| Swift | 00013199005 | 58901 | 2.1 | V(0.17), B(0.17), U(0.17), W1(0.3), M2(0.5), W2(0.7) |
| Swift | 00013199006 | 58907 | 1.9 | V(0.15), B(0.15), U(0.15), W1(0.3), M2(0.47), W2(0.61) |
| eROSITA | eRASS1 | 58911 | 0.3 (0.14) | NONE |
| Swift | 00013199007 | 58912 | 1.2 | V(0.11), B(0.11), U(0.11), W1(0.21), M2(0.22), W2(0.42) |
| Swift | 00013199008 | 58914 | 1.7 | V(0.13), B(0.13), U(0.13), W1(0.26), M2(0.42), W2(0.53) |
| Swift | 00013199009 | 58916 | 1.7 | V(0.14), B(0.14), U(0.14), W1(0.28), M2(0.42), W2(0.56) |
| Swift | 00013199010 | 58919 | 1.7 | V(0.14), B(0.14), U(0.14), W1(0.28), M2(0.42), W2(0.55) |
| eROSITA | eRASS2 | 59093 | 0.3 (0.14) | NONE |
| eROSITA | eRASS3 | 59263 | 0.3 (0.14) | NONE |
| eROSITA | eRASS4 | 59452 | 0.3 (0.14) | NONE |
| Swift | 00014932001 | 59550 | 5.7 | V(0.29), B(0.29), U(0.29), W1(0.85), M2(2.3), W2(1.4) |
| XMM-Newton | 0903991001 | 59651 | 21.0 | V(3.5),B(3.5), W1(4.4), M2(4.4), W2(4.4) |
| Swift | 00015274001 | 59786 | 5.5 | V(0.43), B(0.43), U(0.43), W1(0.87), M2(1.44), W2(1.74) |
| XMM-Newton | 0903991101 | 60017 | 40.0 | V(4.4), B(4.4), U(4.4), M2(4.4) |
Notes. Log of the space-based X-ray, optical, and ultraviolet observations with eROSITA, Swift (XRT and UVOT instruments), and XMM-Newton (EPIC-pn and OM). The exposure times listed in the table for Swift and XMM-Newton are good time intervals (GTI) after screening. For the eROSITA observations we report the GTI and the vignetting-corrected exposure (in parentheses). In this table, W1, M2 and, W2 are abbreviations for the UVW1, UVM2, and UVW2 filters, respectively.
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