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Table 3

X-ray sources detected in the XMM-Newton observation on 1ES 0229+200.

Name Coordinates (J2000) F0.3−12   keV(ergcm-2s-1) Possible counterpart (radio, IR, optical)

1ES 0229+200 02:32:48.592, +20:17:16.15 (3.71 ± 0.04) × 10-11 NVSS 023248+201716, GSC2.2 N3312301936
XMMU 023228.6+202349 02:32:28.690, +20:23:49.10 (2.0 ± 0.2) × 10-12 GSC2.2 N33123012274
XMMU 023227.3+200711 02:32:27.371, +20:07:11.61 (1.2 ± 0.2) × 10-12 NVSS 023227+200711, GSC2.2 N331230310473
XMMU 023147.2+201348 02:31:47.287, +20:13:48.93 (8 ± 2) × 10-13 GSC2.3 NC6R014254
XMMU 023318.0+201237 02:33:18.050, +20:12:37.19 (5 ± 3) × 10-13
XMMU 023212.7+200318 02:32:12.738, +20:03:18.55 (4 ± 2) × 10-13
XMMU 023315.5+201323 02:33:15.554, +20:13:23.39 (4 ± 2) × 10-13 NVSS 023314+201330, IRAS 02304+2000
XMMU 023229.9+200639 02:32:29.933, +20:06:39.66 (3 ± 1) × 10-13 GSC2.2 N331230310392
XMMU 023314.7+200626 02:33:14.715, +20:06:26.90 (2 ± 1) × 10-13
XMMU 023248.2+202858 02:32:48.277, +20:28:58.01 (2 ± 1) × 10-13
XMMU 023315.2+202553 02:33:15.208, +20:25:53.65 (2.1 ± 0.9) × 10-13 GSC2.3 NC6P013245
XMMU 023230.4+201704 02:32:30.426, +20:17:04.60 (2.1 ± 0.5) × 10-13
XMMU 023233.2+200539 02:32:33.215, +20:05:39.75 (2 ± 1) × 10-13 GSC2.3 NC6R010173
XMMU 023219.6+201201 02:32:19.684, +20:12:01.90 (1.6 ± 0.9) × 10-13 NVSS 023219+201204
XMMU 023323.5+202140 02:33:23.568, +20:21:40.04 (1.6 ± 0.8) × 10-13 GSC2.3 NC6P013116
XMMU 023321.4+202330 02:33:21.475, +20:23:30.11 (1.2 ± 0.6) × 10-13 GSC2.3 NC6P002203
XMMU 023314.7+200852 02:33:14.791, +20:08:52.69 (0.3 ± 1) × 10-13 GSC2.3 NC6R010904
XMMU 023254.6+202352 02:32:54.603, +20:23:52.74 (9 ± 5) × 10-14
XMMU 023307.2+201040 02:33:07.248, +20:10:40.15 (8 ± 4) × 10-14 GSC2.3 NC6R011298
XMMU 023328.0+202342 02:33:28.066, +20:23:42.91 (8 ± 6) × 10-14 IRAS 02306+2010
XMMU 023310.8+201929 02:33:10.871, +20:19:29.55 (5 ± 3) × 10-14 GSC2.3 NC6P001373
XMMU 023211.7+201721 02:32:11.773, +20:17:21.75 (1 ± 3) × 10-14 GSC2.2 N3312301924

Notes. Their possible counterparts in the radio, IR, and optical regimes were searched in the Guide Star Catalog (GSC) (Lasker et al. 2008), the IRAS faint source catalog (Moshir 1990), and the NRAO VLA Sky Survey (NVSS) (Condon et al. 1998).

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