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Table 2

XMM-Newton imaging observations of (c)LBVs.

Simbad name Obsid Rev. OFA EPIC count rate log  [LX/LBOL] 
(′) ct s-1 erg cm-2 s-1 erg s-1
P Cyg 0600030201 1891 0.  <0.0010  <1.0 × 10-15  <8.3 × 1029  <−9.4
AG Car 0600030101 1853 0.  <0.0009  <8.1 × 10-16  <1.0 × 1031  <−8.7..8.8
HD 160529 0600030701 1797 0.  <0.0008  <7.8 × 10-16  <3.2 × 1030  <−8.5
GAL 024.73+00.69 0301880301 1145 5.6  <0.006  <8.4 × 10-15  <7.2 × 1032  <−6.3
Cl* Westerlund 1 W 243 0410580601 1317 0.5  <0.0017  <2.6 × 10-15  <2.3 × 1032  <−7.1
0505290201 1409 0.5
0505290301 1499 0.5
0555350101 1593 0.5
0604380101 1778 0.5
HD 316285 0112970101 0145 7.8  <0.0013  <1.4 × 10-15  <6.1 × 1030  <−8.2
GRS 25.5+0.2 0400910301 1256 10.  <0.0025  <5.7 × 10-15  <1.7 × 1034
NAME LBV 1806-20a 0205350101 0869 0.  <0.01  <2.2 × 10-14  <4.1 × 1034  <−5.3
0164561101 0884 0.
0164561401 1066 0.
0406600301 1157 0.
0406600401 1237 0.
0502170301 1428 0.
0502170401 1523 0.
0554600301 1601 0.
0554600401 1691 0.
MCW 930b 0650591501 2059 7.5  <0.0006  <1.9 × 10-15  <5.0 × 1031  <−7.4
2MASS J17110094–3945174 0502080301 1431 0.9  <0.003  <3.2 × 10-15
2MASS J16461734–4508478 0164561001 0873 2.6  <0.004  <4.9 × 10-15
2MASS J18022233–2238002 0135742801 0600 11.  <0.0035  <3.8 × 10-15
MN53b 0148690101 0681 6.9  <0.0005  <1.5 × 10-15
MN79 0051940401 0229 3.7  <0.0012  <1.3 × 10-15
eta Car see Corcoran et al. (2010) 0.06..3 × 10-10  ~–5
NAME VI Cyg 12 see Rauw (2011) 2.7 × 10-12 8.2 × 1033 −6.1

Notes. A null off-axis angle (OFA) indicates an on-axis observation. Column 1 provides the (c)LBV name, Cols. 2 to 4 the details of the observation(s) used, and the next columns list the derived EPIC count rates, fluxes, and luminosities in the 0.5–8.0 keV energy range. Limits correspond to a 90% chance of being detected if brighter.

(a)

Three additional observations (Obsid – Rev = 0148210101 – 0607, 0148210401 – 0701, and 0164561301 – 0960) are available but are totally affected by strong flares: they were therefore discarded from the analysis.

(b)

Refers to EPIC MOS data only.

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