IPs

V455 And
V515 And
AE Aqr
FO Aqr
XY Ari
V405 Aur
V647 Aur
HT Cam
MU Cam
DW Cnc
BG CMi
V709 Cas
V1033 Cas
V1025 Cen
TV Col
TX Col
UU Col
V2069 Cyg
V2306 Cyg
YY Dra
PQ Gem
V418 Gem
DQ Her
V1323 Her
EX Hya
NY Lup
V2400 Oph
V2731 Oph
V598 Peg
GK Per
AO Psc
V667 Pup
WX Pyx
V1223 Sgr
CC Scl
V1062 Tau
EI UMa
AX J1740.1
AX J1740.2
AX J1853.3
IGR J08390
IGR J15094
IGR J16500
IGR J16547
IGR J17195
IGR J18173
IGR J18308
IGR 19267
RX J2133

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Revnivtsev et al. 2008

Bibinfo (this paper at ADS)
Revnivtsev, M., Sazonov, S., Krivonos, R., Ritter, H., Sunyaev, R. 2008, A&A, 489, 1121-1127.
Type
Observational: Analysis of INTEGRAL survey sample.
Object(s):
14 IPs and candidates (V709 Cas, V2069 Cyg, NY Lup, V2400 Oph, V2487 Oph, GK Per, V1223 Sgr, V2731 Oph, V1062 Tau, IGR J15094-6649, IGR J16167-4957, IGR J16500-3307, and IGR J17195-4100, 1RXS J213344.1+510725,) as wel as V1432 Aql, IGR J14536-5522, and SS Cyg.
Results
The authors start with the dubious assumption that the distances to 5 IPs and 1 polar in the sample are securely known (only one of the 6 is in fact secure) and purport to derive the spatial distribution and the X-ray luminosity function of hard X-ray emitting CVs.


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