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

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arxiv 2401.11931 v1 pith:HKEHYJ3Z submitted 2024-01-22 astro-ph.HE

classification astro-ph.HE
keywords lmxbscataloguex-raybinariesdetectedinformationparametersbuild
verification ladder T0 review T1 audit T2 compute T3 formal
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Low-mass X-ray binaries (LMXBs) are high-energy sources that require multi-wavelength follow up campaigns to be fully characterized. New transients associated to 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 up to a useful tool for subsequent studies on LMXBs and their population. We provide an update on past LMXB catalogues dating back 16 years 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 to host 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. We build a working base by cross-matching previous LMXB catalogues and supplementing them with lists of hard X-ray sources detected in the past 20 years. We compile 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 retrieve newly detected LMXBs and candidates directly from literature searches. Counterparts to these LMXBs are compiled from hard X-rays to infrared and radio domains. Every piece of information presented on the LMXBs is curated and backed by accurate references. 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 {\it Gaia} DR3.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Resolving SLX 1744-299 and SLX 1744-300 in the hard X-ray band: implications for their ultracompact nature

    astro-ph.HE 2026-06 unverdicted novelty 6.0 of 10

    NuSTAR resolves SLX 1744-299 and SLX 1744-300 in hard X-rays, yielding low luminosities that favor ultracompact orbital periods below 90-155 min via disc instability model comparison.

  2. An Elaborate Search for Coherent Pulsations from Intermittent-AMXPs

    astro-ph.HE 2025-02 conditional novelty 5.0 of 10

    A systematic Z1^2 and maximum-likelihood search of RXTE data finds dozens of intermittent pulse candidates in three accreting millisecond pulsars and derives an 8.76 h orbital period for SAX J1748.9-2021.

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