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Table 4

Faint SSS candidates in the SMC.

No. RAa Deca ePosb H R 1 H R 2 F c M L det d M L pn d M L m1 d M L m2 d Comment

235 01 01 47.58 −71 55 50.7 0.85 −0.3 ± 0.1 −0.8 ± 0.1 6.0 ± 0.6 146.5 54.7 33.2 4.2 WD/Be?
1198 01 01 24.19 −72 00 37.9 1.82 −0.4 ± 0.2 −1.0 ± 0.5 2.5 ± 0.7 16.2 9.4 6.2 2.8
1531 00 39 45.58 −72 47 01.4 1.58 −1.0 ± 0.1 0.8 ± 0.4 1.8 ± 0.4 28.6 10.7 7.8 12.2 star?
1549 00 38 58.74 −72 55 10.4 1.68 −1.0 ± 0.2 3.6 ± 0.9 18.3 13.6 4.5 2.9 star?
2132 00 57 45.29 −71 45 59.7 0.93 −0.4 ± 0.1 −0.5 ± 0.2 4.1 ± 0.5 121.1 85.4 20.4 18.8
2178 00 55 37.71 −72 03 14.0 0.74 −0.9 ± 0.0 0.2 ± 0.4 6.7 ± 0.5 391.5 282.6 54.5 58.7
2218 00 55 08.45 −71 58 26.7 1.38 −0.2 ± 0.2 −0.9 ± 0.4 1.3 ± 0.3 14.0 13.0 3.2 0.9 WD/Be?, star?
3235 00 55 03.65 −73 38 04.1 0.64 −0.9 ± 0.0 0.2 ± 0.2 13.6 ± 0.8 787.0 649.0 48.1 96.2

Notes.

(a)

Sexagesimal coordinates in J2000.

(b)

Positional uncertainty in arcsec.

(c)

Detected flux in the (0.2−1.0) keV band in 10-15 erg cm-2 s-1.

(d)

Source detection likelihood for combined and the individual instruments.

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