V455 And
V515 And
AE Aqr
FO Aqr
V349 Aqr
XY Ari
V405 Aur
V647 Aur
HT Cam
MU Cam
DW Cnc
V709 Cas
V1025 Cen
V1033 Cas
TV Col
TX Col
UU Col
V2069 Cyg
V2306 Cyg
DO Dra
PQ Gem
V418 Gem
DQ Her
V1323 Her
V1460 Her
V1674 Her
EX Hya
NY Lup
V2400 Oph
V2731 Oph
V3037 Oph
V598 Peg
GK Per
AO Psc
HZ Pup
V667 Pup
WX Pyx
V1223 Sgr
V4743 Sgr
CC Scl
V1062 Tau
AX J1740.1
AX J1832.3
AX J1853.3
CTCV J2056
CXO J174954
IGR J04571
IGR J08390
IGR J15094
IGR J16500
IGR J16547
IGR J17014
IGR J17195
IGR J18151
IGR J18173
IGR J18308
IGR J19267
PBC J0927.8
PBC J1841.1
RX J1804
RX J2015
RX J2113
RX J2133
RX J2306
Swift J0717
Swift J1839
Swift J2006
Swift J2138

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Thorstensen & Halpern 2013

Bibinfo (this paper at ADS)
Thorstensen, J.R., Halpern, J., 2013, AJ, 146, A107 (19 pp.).
Observational: Optical spectroscopy & photometry.
V3037 Oph, V667 Pup, IGR J04571+4527, Swift J0746.2-1611, IGR J18173-2509, IGR J18308-1232 AX J18533-0128, IGR J19267+1325, and IGR J19552+0044, as well as the polar Swift J2218.4+1925.
Optical spectroscopy of 10 hard X-ray discovered CVs has resulted in the secure orbital period determination for 8, and candidate periods for the remaining two. Of these, 7 show coherent pulsations either in the X-rays and/or the optical, and are identified as IPs. Swift J0757.2-1611 is a nova-like which could be an IP (but so far, there is no evidence for its spin period), IGR J19552+0044 is an unusual object, while Swift J2218.4+1925 is a polar.

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