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Table 3.

Intermediate polars used by Pretorius & Mukai (2014) to obtain the space density.

Name (pc) fX (erg cm−2 s−1) p (mas) Δp (mas) log LX (s−1) D (pc) Dmax (pc) Vgen (pc3)
V1223 Sgr 527 33.6 1.18E–10 1.725 0.047 33.7 571 1241 1.22E+09
V2400 Oph 280 32.7 5.00E–11 1.399 0.033 33.5 701 991 1.51E+09
AO Psc 330 32.6 3.20E–11 2.021 0.043 33.0 488 552 5.48E+07
IGR J16500 430 32.8 2.60E–11 0.855 0.062 33.6 1140 1163 2.46E+09
V405 Aur 380 32.8 3.50E–11 1.487 0.031 33.3 662 783 5.78E+08
FO Aqr 450 33.1 5.20E–11 1.902 0.051 33.2 518 747 7.76E+07
PQ Gem 510 33.0 3.10E–11 1.306 0.036 33.3 750 835 4.28E+08
TV Col 368 33.0 6.00E–11 1.951 0.018 33.3 505 782 1.94E+08
IGR J15094 960 33.5 2.60E–11 0.859 0.028 33.6 1127 1149 2.35E+09
XY Ari 270 32.5 3.60E–11 3.700 1.500 32.5 270 324 4.33E+07
EI UMa 750 33.3 2.90E–11 0.883 0.037 33.6 1095 1179 1.66E+08
NY Lup 680 33.7 9.20E–11 0.786 0.028 34.2 1228 2356 9.38E+09
V1062 Tau 1400 33.8 2.50E–11 0.632 0.077 33.8 1512 1512 2.72E+09
V2731 Oph 1000 33.9 6.90E–11 0.436 0.056 34.6 2165 3597 2.25E+09
GK Per 477 33.3 7.80E–11 2.263 0.043 33.3 437 772 7.74E+08

Notes. The luminosity is given in the spectral band 14–195 keV. Distances and luminosities with tildes are from the orginal publication, those without are from this work. Vgen was computed for a scale height of 120 pc.

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