V455 And
V515 And
AE Aqr
FO Aqr
XY Ari
V405 Aur
V647 Aur
HT Cam
MU Cam
DW Cnc
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
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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Scaringi et al. 2010

Bibinfo (this paper at ADS)
Scaringi, S., Bird, A.J., Norton, A.J., Knigge, C., Hill, A.B., Clark, D.J., Dean, A.J., McBride, V.A., Barlow, E.J., Bassani, L., Bazzano, A., Fiocchi, M., Landi, R. 2010, MNRAS, 401, 2207-2218.
Observational: Hard X-rays.
Confirmed IPs AE Aqr, FO Aqr, XY Ari, V405 Aur, MU Cam, BG CMi, V709 Cas, V1033 Cas, TV Col, TX Col, V2069 Cyg, YY Dra, PQ Gem, EX Hya, NY Lup, V2400 Oph, V2731 Oph, GK Per, AO Psc, V667 Pup, and V1223 Sgr, V1062 Tau, IGR J08390-4833, IGR J16500-3307, IGR J15094-6649, IGR J17195-4100, and 1RXS J213344.1+510725; Candidade IPs TW Pic, IGR J16167-4957, V2487 Oph, IGR J18173-2509, IGR J18303-1232, AX J1832.3-0840, and IGR J19267+1325; Polars BY Cam, V834 Cen, IGR J14536-5522, and V1432 Aql; as well as SS Cyg and XSS J12270-4859.
IBIS catalog and Swift/BAT and Suzaku/HXD observations are used to study the population of hard X-ray emitting megnetic CVs. Correlation between hard X-ray hardness and spin-to-orbital period ratio is found in the sample.

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