Multiwavelength Characterization of a New Magnetic Cataclysmic Variable 2CXO J050740.7-091337
Ilkham Galiullin, Vladislav Dodon, Antonio C. Rodriguez, Paula Szkody, and Askar Sibgatullin

TL;DR
This paper reports the discovery and detailed multiwavelength characterization of a new magnetic cataclysmic variable, 2CXO J0507, highlighting its properties and significance for future surveys.
Contribution
It presents the first identification and analysis of 2CXO J0507, a faint magnetic CV, using X-ray, optical, and archival data, emphasizing its relevance for upcoming large-scale surveys.
Findings
2CXO J0507 is a strongly magnetized white dwarf with B ≈ 30 MG.
X-ray luminosity is approximately 5.18 × 10^{30} erg s^{-1}.
Orbital period is estimated at 2.34 hours.
Abstract
We report the discovery and characterization of a new cataclysmic variable (CV), 2CXO J050740.7-091337 (hereafter 2CXO J0507), identified using the X-ray main sequence through a cross-match between the Chandra Source Catalogue 2.1 and Gaia DR3. Optical spectroscopic follow-up with Keck I/LRIS reveals prominent cyclotron humps and Balmer emission lines, indicating a strongly magnetized white dwarf with a magnetic field strength of MG. Analysis of Chandra and XMM-Newton archival data shows an X-ray luminosity of erg s (0.3-10 keV). The X-ray spectrum is well approximated by a thermal plasma emission model with a temperature of keV, showing no soft excess or intrinsic absorption. 2CXO J0507 exhibits long-term optical variability by mag (ranging mag) in Zwicky Transient…
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