On the use of field RR Lyrae as Galactic probes: VII. Light curve templates in the LSST photometric system
Context. The Vera C. Rubin Observatory will start operations in 2025. During its first two years, too few visits per target per band will be available, meaning that the mean magnitude measurements of variable stars will not be precise and thus standard candles such as RR Lyrae (RRL) will not be usable. Light curve templates (LCTs) can be adopted to
Braga, V. F. et al.
Fecha de publicación:
9
2024