Deep Optical Photometry of Six Fields in the Andromeda Galaxy
Thomas M. Brown, Ed Smith, Henry C. Ferguson (STScI), Puragra, Guhathakurta (UCO/Lick), Jason S. Kalirai (STScI), Randy A. Kimble (GSFC),, Alvio Renzini (INAF), R. Michael Rich (UCLA), Allen V. Sweigart (GSFC), Don, A. VandenBerg (UVic)

TL;DR
This study provides deep optical imaging of six fields in the Andromeda Galaxy using Hubble, enabling detailed analysis of its stellar populations and star formation history.
Contribution
First deep optical photometry reaching below the oldest main sequence turnoff in multiple Andromeda fields, with data and catalogs made publicly available.
Findings
High-quality images and catalogs of six Andromeda fields
Artificial star tests for completeness and photometric accuracy
Data supporting star formation history analysis
Abstract
Using the Advanced Camera for Surveys on the Hubble Space Telescope, we have obtained deep optical images reaching well below the oldest main sequence turnoff in six fields of the Andromeda Galaxy. The fields fall at four positions on the southeast minor axis, one position in the giant stellar stream, and one position on the northeast major axis. These data were obtained as part of three large observing programs designed to probe the star formation history of the stellar population in various structures of the galaxy. In this paper, we present the images, catalogs, and artificial star tests for these observing programs as a supplement to the analyses published previously. These high-level science products are also archived at the Multimission Archive at the Space Telescope Science Institute.
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.
