Table 1

X-ray sources detected within the Hoinga SNR in eROSITA eRASS1 and ROSAT RASS data.

Source RA (J2000) Dec (J2000) Obs. time
h:m:s d:m:s ⟨MJD⟩
eROSITA eRASS1

1 09:33:41.096 −17:09:18.932 58 987.40282
2 09:33:18.088 −17:14:41.741 58 987.31946
3 09:34:30.071 −17:21:21.224 58 987.65274
4 09:37:57.489 −17:10:14.453 58 988.23630
5 09:27:29.469 −18:06:20.653 58 986.48550
6 09:27:50.522 −16:40:01.672 58 985.98614
7 09:36:25.814 −18:21:05.829 58 988.40257
8 09:28:45.469 −15:24:10.805 58 985.73667
9 09:28:38.097 −15:21:08.361 58 985.73682
10 09:40:02.199 −17:09:55.614 58 988.65310
11 09:26:58.572 −16:30:06.584 58 985.73626

ROSAT RASS

1 09:33:41.421 −17:08:59.602 48 210.59365
2 09:33:18.151 −17:14:39.386 48 210.52687
3 09:34:30.177 −17:21:17.739 48 210.86065
4 09:37:57.671 −17:10:07.991 48 211.72799
7 09:36:26.231 −18:21:05.791 48 211.82793
10 09:40:02.494 −17:09:58.469 48 212.26215
11 09:26:58.256 −16:30:01.930 48 208.55845

Notes. The detection significance of the listed sources is ≥5σ. The position uncertainty of eROSITA point sources is 4.′′5 (1σ confidence). ⟨MJD⟩ is the Modified Julian Date of the observation in eRASS1 and RASS, respectively. The numbering for the centrally located sources #1 − #3 is reported in the lower-right inset of Fig. 3.

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