AstroSat UVIT Survey of M31: New Compact Source Catalog
Denis Leahy, Sujith Ranasinghe, Saptadwipa Mitra, Kripansh Rawal

TL;DR
This paper presents a comprehensive ultraviolet survey of M31 using AstroSat's UVIT instrument, resulting in a new, extensive catalog of over 115,000 sources with improved detection sensitivity and spatial resolution.
Contribution
The study provides the largest and most sensitive UV source catalog for M31 to date, with enhanced data processing and additional observations compared to previous catalogs.
Findings
Detected over 115,000 sources in UV wavelengths.
Achieved a magnitude limit of approximately 23.0 in F148W band.
Produced a detailed catalog with positions, fluxes, and magnitudes.
Abstract
An ultraviolet survey of M31 has been carried out during 2017-23 with the UVIT instrument onboard the AstroSat Observatory. Here we present far and near ultraviolet (FUV and NUV) observations from the M31 UVIT survey, which covers a sky area of with spatial resolution of . The observations included six filter bands in the wavelength range of 120 nm to 280 nm. Including the six bands, 115,000 sources with signal-to-noise S/N3 ( 95,000 sources with signal-to-noise S/N5) were detected at FUV or NUV wavelengths, with the largest set of detections (54,000 sources) in the FUV 150 nm band (F148W filter). This is considerably more than for the first version of the M31 source catalog (published in 2020), in part due to additional observations of M31 by UVIT and in part due to improved data processing.…
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.
Taxonomy
TopicsAstronomy and Astrophysical Research · Astronomical Observations and Instrumentation · Stellar, planetary, and galactic studies
