arXiv (All)
open access
Beyond what's observed: hierarchical inference of Gaia astrometric compact-object binaries
Astrometry from the Gaia mission has revealed a large and homogeneous population of binaries containing compact objects, including more than 3000 white dwarf--main sequence (WDMS) binaries with orbital periods of $P_{\rm orb}\sim100$--$1000$ d. Most of these binaries likely underwent mass transfer f
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- A Sample of Long-Period Binaries with Dormant Compact-Object Candidates from LAMOST DR13 MRS and Gaia DR3#1105323
- Strong constraints on the gravitational law from $Gaia$ DR3 wide binaries#1128487
- Companion masses of Gaia DR3 AstroSpectroSB1 binaries: a Bayesian forward-modelling framework#1050501
- An unresolved extreme warm infrared excess toward a nearby low-mass star#1000008
- Closed-Form of the Local Galactic Potential and Stellar Distribution Function from Gaia DR3#986623
Record · ID 1130841
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive