A catalogue of low-mass X-ray binaries in the Galaxy: From the INTEGRAL to the Gaia era^★

¹ IRAP, Université de Toulouse, CNRS, CNES, UPS, 31401 Toulouse, France
e-mail: francis.fortin@irap.omp.eu
² Université Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France
³ Delhi Technological University, Delhi 110042, India
⁴ Department of Physics and Astronomy “Galileo Galilei”, University of Padua, Padua, Italy
⁵ Instituto Argentino de Radioastronomía, CCT La Plata, CONICET; CICPBA; UNLP, C.C.5, 1894 Villa Elisa, Buenos Aires, Argentina

Received: 8 September 2023
Accepted: 22 January 2024

Abstract

Context. Low-mass X-ray binaries (LMXBs) are high-energy sources that require multi-wavelength follow-up campaigns to be fully characterised. New transients associated with LMXBs are regularly discovered, and previously known systems are often revisited by astronomers to constrain their intrinsic parameters. All of this information compiled into a catalogue may build a useful tool for subsequent studies on LMXBs and their population.

Aims. We aim to provide an update on past LMXB catalogues dating back 16 yr and propose to the community a database on Galactic LMXBs with the most complete, manually curated set of parameters and their original references. On top of a fixed version accessible through Vizier, we propose hosting the catalogue independently on our GitHub collaboration, side-by-side with our previous catalogue on high-mass X-ray binaries. The database will be regularly updated based on new publications and community inputs.

Methods. We built a working base by cross-matching previous LMXB catalogues and supplementing them with lists of hard X-ray sources detected over the past 20 yr. We compiled information from Simbad on LMXBs as a starting point for a thorough, manual search in the literature to retrieve important parameters that characterize LMXBs. We retrieved newly detected LMXBs and candidates directly from literature searches. Counterparts to these LMXBs are compiled from hard X-ray to infrared and radio domains. Every piece of information presented on the LMXBs is curated and backed by accurate references.

Results. We present a catalogue of 339 Galactic LMXBs listing their coordinates, companion star spectral type, systemic radial velocity, component masses and compact object nature, the presence of type I X-ray bursts, as well as orbital data. Coordinates and identifiers of counterparts at various wavelengths are given, including 140 LMXBs detected in Gaia DR3.