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Table 1

Additional X-ray sources in the XMM-Newton M 31 survey catalogue of Stiele et al. (2011) analysed in this work.

[SPH11] RA (2000.0) Dec (2000.0) Pos. error Rate MLa H R1b H R2b H R3b H R4b
ID [arcsec] [cts/s]
Additional SNR candidates

811 00 42 10.60 +40 51 49.1 6.19 3.0e–3  ±  1.0e–4 8.3 –0.46  ±  0.46 0.48  ±  0.46 –0.83  ±  0.36
833 00 42 14.60 +40 52 04.7 4.30 3.2e–3  ±  5.0e–5 26 0.73  ±  0.17 –0.09  ±  0.17 –0.84  ±  0.23
c1121 00 43 03.70 +41 37 17.2 4.47 5.4e–3  ±  1.0e–4 17 0.45  ±  0.24 0.14  ±  0.19 –0.23  ±  0.36
1286 00 43 42.08 +41 47 09.5 7.42 2.2e–3  ±  5.0e–5 8.6 0.74  ±  0.27 –0.38  ±  0.23 –0.85  ±  0.46
d1461 00 44 28.62 +41 49 48.7 7.00 2.7e–3  ±  7.0e–5 8.7 0.63  ±  0.33 –0.58  ±  0.29
c1468 00 44 30.56 +41 23 06.2 4.84 4.0e–3  ±  6.0e–5 38 0.82  ±  0.16 0.16  ±  0.17 –0.66  ±  0.30
c1611 00 45 18.44 +41 39 36.3 3.42 7.5e–3  ±  8.0e–5 94 0.85  ±  0.17 0.29  ±  0.11 –0.13  ±  0.14

Notes. Sources in this table have been studied as possible SNR candidates based on optical data (see Sect. 2.1).

(a)

Detection likelihood.

(b)

Hardness ratios.

(c)

Classified as a hard source by SPH11.

(d)

Classified as a foreground star candidate by SPH11.

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