The impact of Gaia and LSST on binary stars and exo-planets
L. Eyer, P. Dubath, N. Mowlavi, P. North, A. Triaud, F. Barblan, C., Siopis, L. Guy, B. Tingley, S. Zucker, D. W. Evans, L. Wyrzykowski, M., Suveges, Z. Ivezic
TL;DR
Gaia and LSST will revolutionize the study of binary stars and exoplanets by providing vast data sets through astrometry, photometry, and radial velocity, enabling new discoveries and tools.
Contribution
This paper reviews potential tools and scientific gains from Gaia and LSST data for binary and exoplanet research, highlighting their expected impact.
Findings
Millions of binary systems will be observed by Gaia.
Tens of millions of systems will be detected by LSST.
Enhanced detection and characterization methods will be developed.
Abstract
Two upcoming large scale surveys, the ESA Gaia and LSST projects, will bring a new era in astronomy. The number of binary systems that will be observed and detected by these projects is enormous, estimations range from millions for Gaia to several tens of millions for LSST. We review some tools that should be developed and also what can be gained from these missions on the subject of binaries and exoplanets from the astrometry, photometry, radial velocity and their alert systems.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.