Ultracool Dwarf Science from Widefield Multi-Epoch Surveys
N.R. Deacon (1), D.J. Pinfield (2), P.W. Lucas (2), Michael C. Liu, (1), M.S. Bessell (3), B. Burningham (2), M.C. Cushing (4), A.C. Day-Jones, (5), S. Dhital (6), N.M. Law (7), A.K. Mainzer (4), Z.H. Zhang (2) ((1), Institute for Astronomy, University of Hawai`i
TL;DR
This paper discusses how new multi-epoch widefield surveys enhance the study of ultracool dwarfs by providing deeper data and enabling time-domain analysis, building on previous single-epoch surveys.
Contribution
It introduces the potential of multi-epoch surveys to advance ultracool dwarf research through increased depth and temporal coverage.
Findings
Multi-epoch surveys enable time-domain studies of ultracool dwarfs.
Deeper surveys expand the parameter space for ultracool dwarf detection.
New surveys complement previous single-epoch data, opening new research avenues.
Abstract
Widefield surveys have always provided a rich hunting ground for the coolest stars and brown dwarfs. The single epoch surveys at the beginning of this century greatly expanded the parameter space for ultracool dwarfs. Here we outline the science possible from new multi-epoch surveys which add extra depth and open the time domain to study.
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Astronomical Observations and Instrumentation