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Table A.1

Flux-limited sample: 33 sources from the RXTE Slew Survey with a count rate in the 3–8 keV energy range greater than 1 cts/sec and fulfilling the FERO source selection criteria.

Source Type RXTE slew survey XMM-Newton XMM-Newton exposure time
(cts/s)3−8 keV (cts/s)2−10 keV (ks)

NGC 4593 BLSY 1.05  ±  0.16 4.613  ±  0.009 53.2
MRK 704 BLSY 1.06  ±  0.22 0.984  ±  0.009 14.9
ESO511-G030 NCSY 1.10  ±  0.09 2.284  ±  0.005 76.2
NGC 7213 BLSY 1.12  ±  0.16 2.448  ±  0.009 29.6
AKN 564 NLSY 1.13  ±  0.02 2.246  ±  0.005 84.1
H1846-786 NCSY 1.15  ±  0.09 0.700  ±  0.011 6.3
MRK 110 NLSY 1.17  ±  0.10 3.362  ±  0.010 32.8
ESO198-G024 BLSY 1.21  ±  0.19 1.150  ±  0.003 85.3
FAIRALL9 BLQ 1.25  ±  0.02 1.313  ±  0.007 25.9
UGC 3973 BLSY 1.32  ±  0.12 1.304  ±  0.019 3.6
NGC 4051 NLSY 1.49  ±  0.02 2.783  ±  0.007 73.3
NGC 526A NCSY 1.61  ±  0.14 2.177  ±  0.007 41.5
MCG-2-58-22 BLSY 1.61  ±  0.08 3.459  ±  0.021 7.2
NGC 7469 BLSY 1.69  ±  0.01 3.343  ±  0.005 142.6
MRK 766 NLSY 1.77  ±  0.12 1.962  ±  0.002 398.3
MRK 590 BLSY 1.95  ±  0.10 0.766  ±  0.003 72.0
IRAS05078+1626 NCSY 2.08  ±  0.19 2.691  ±  0.008 40.1
NGC 3227 BLSY 2.10  ±  0.02 3.635  ±  0.006 97.4
MR2251-178 BLQ 2.10  ±  0.11 2.387  ±  0.007 44.5
MRK 279 BLSY 2.13  ±  0.06 3.110  ±  0.006 104.8
ARK 120 BLSY 2.14  ±  0.03 4.553  ±  0.008 76.3
NGC 7314 NCSY 2.16  ±  0.04 4.509  ±  0.012 30.1
H0557-385 NCSY 2.33  ±  0.34 4.254  ±  0.021 10.5
MCG+8-11-11 BLSY 2.36  ±  0.27 4.838  ±  0.014 26.5
MCG-6-30-15 BLSY 3.08  ±  0.02 4.719  ±  0.004 295.1
MRK 509 BLQ 3.12  ±  0.10 4.432  ±  0.005 27.8
NGC 3516 BLSY 3.21  ±  0.01 1.841  ±  0.004 153.0
NGC 5548 BLSY 3.58  ±  0.02 4.191  ±  0.007 74.8
NGC 3783 BLSY 4.90  ±  0.04 5.539  ±  0.006 170.4
MCG-5-23-16 NCSY 6.46  ±  0.12 8.025  ±  0.008 110.3
IC 4329A BLSY 7.29  ±  0.07 10.713  ±  0.011 85.1

UGC10683 SY 1.27  ±  0.18
ESO141-G055 SY 1.37  ±  0.12

Notes. These sources, with the exception of the last two sources, have all been the target of XMM-Newton observations. The XMM-Newton EPIC-pn count rate in the 2–10 keV energy range and exposure time is also given. For two of them, UGC 10683 and ESO 0141-G055, no XMM-Newton data were available as of April 2008. This reduces the number of XSS-selected bright sources in the FERO sample to 31.

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