Recognition: unknown
A Higher Cadence Subsurvey Located in the Galactic Plane
classification
🌌 astro-ph.IM
astro-ph.EPastro-ph.SR
keywords
galacticplanecadencehigherobservationssourceswilladdress
read the original abstract
Presently, the Galactic plane receives relatively few observations compared to most of the LSST footprint. While this may address static science, the plane will also represent the highest density of variable Galactic sources. The proper characterization of variability of these sources will benefit greatly from observations at a higher cadence.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.