arXiv (All)
open access
A pilot study on the CSST astrometric capability: Detecting astrometric binaries with Gaia synergy via simulated data
Context. The China Space-station Survey Telescope (CSST) will provide deep, wide-field epoch astrometry during its 10-year mission. Astrometric binary orbits constrain the masses of stellar and compact-object components. Orbital recovery depends on astrometric precision and temporal coverage. Combin
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
- Gaia DR3 Limits on Stellar Engine Technosignatures in Nearby Stars#620480
- Gaia DR3 Limits on Stellar Engine Technosignatures in Nearby Stars#618801
- Challenging the archetypal intermittent radio galaxy J0111+3906. New insights from optical GTC/OSIRIS and radio VLA and LOFAR observations#1012722
- Bayesian analysis of Gaia epoch astrometry and radial velocities with kima#985146
- Additional values from the SPARV pipeline#934105
Record · ID 987967
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