National Aeronautics and Space Administration

IPs

V455 And
V515 And
AE Aqr
FO Aqr
V349 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
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
EI UMa
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
LAMOST 0240
PBC J0927.8
PBC J1841.1
RX J1804
RX J2015
RX J2113
RX J2133
RX J2306
Swift J0717
Swift J1839
Swift J2006
Swift J2138

Full Catalog

Related Systems

Suleimanov, Doroshenko & Werner 2022

Bibinfo (this paper at ADS)

Suleimanov, V.F., Doroshenko, V., Werner, K., 2022, MNRAS, 511, 4937-4945.

Type

Observational: Hard X-ray luminosity funciton.

Object(s)

V515 And, FO Aqr, V405 Aur, V647 Aur, MU Cam, BG CMi, V709 Cas, V1033 Cas, V1025 Cen, TV Col, TX Col, V2069 Cyg, V2306 Cyg, DO Dra, PQ Gem, V418 Gem, EX Hya, NY Lup, V2400 Oph, V2731 Oph, GK Per, AO Psc, V667 Pup, V1223 Sgr, V1062 Tau, EI UMa, AX J1832.3-0840, IGR J04571+4527, IGR J08390-4833, IGR J15094-6649, IGR J16500-3307, IGR J16547-1916, IGR J17014-4306, IGR J17195-4100, IGR J18151-1052, IGR J18173-2509, IGR J18308-1232, PBC J0927.8-6945, 1RXS J211336.1+542226, 1RXS J213344.1+510725, Swift J0503.7-2819, Swift J0717.8-2156, and Swift J2006.4+3645 among ironclad or confiremd IPs, V1082 Sgr, IGR J14257-6117, Paloma, Swift J0525.6+2416, Swift J0535.2+2830, Swift J0614.0+1709, and Swift J0958.0-4208, among probable IPs, and TW Pic, IGR J12123-5802, IGR J16167-4957, Swift J0746.3-1611, and Swift J2237.2+6324, among possible IPs. Also included are objects that are unlikely to be IPs, such as polars (including asynchronous polars) and candidate polars V1432 Aql (AP), BY Cam (AP), V834 Cen, IW Eri, YY Sex, AM Her, CD Ind (AP), V2301 Oph, IGR J14536-5522, IGR J19552+0044 (AP), Swift J0706.8+0325, Swift J2218.4+1925, Swift J2319.4+2619, and Swift J2341.0+7645; dwarf novae Z Cam, HL CMa, SS Cyg, V426 Oph, and RU Peg; nova-likes AH Men, V2487oph (long orbital period object), V603 Aql (AP), and Swift J0623.9-0939 (long orbital period object),

This paper also associates SWIFT J0612.2-4645 with V347 Pup, even though these objects are almost 2 degress apart; the BAT source appears to be associated with the AGN, PMN J0612-4647.

Also mentioned in this papers are objects without Gaia distances or whose Gaia distances were unknown to the authors. XY Ari (ironclad IP), IGR J14091-6108 (probable IP), possible IPs IGR J12134-6015, 2PBC J0800.5-4306, PBC J0826.3-7033, Swift J0749.7-3218, and Swift J0939.76-3224, as well as Swift J0820.6-2805 whose IP credential is considered doubtful.

Results

BAT detected CVs with X-ray luminosities above 10³³ erg/s are predominantly IPs, while other subclasses dominates at lower luminosities.