A Uniform Census of Variable Stars in M101 Based on HST/ACS Photometry

arXiv:2609.05825 · astro-ph.SR, astro-ph.GA · Submitted 2026-09-05 · Read on arXiv

astro-ph.SR, astro-ph.GA

Submitted: 2026-09-05

Updated: 2026-09-05

Comments: 16 pages, 6 figures, 4 tables; accepted for publication in ApJ

License: http://creativecommons.org/licenses/by/4.0/

The gist: We present a homogeneous HST/ACS F555W/F814W time-series census of variable stars in two M101 disk fields, using a uniform multi-band reduction and reproducible variable-selection workflow for nearby

Terminology

Abstract

We present a homogeneous HST/ACS F555W/F814W time-series census of variable stars in two M101 disk fields, using a uniform multi-band reduction and reproducible variable-selection workflow for nearby SN-host galaxies. Supplementary archival F555W epochs are used only to refine selected long-period solutions. Candidates are selected with Lomb-Scargle period searches, Fourier light-curve modeling, two-band consistency statistics, artificial-star-test photometric corrections, and mode-aware Cepheid refinement. The final catalog contains 1417 variable-star candidates, including 1102 secure fundamental-mode and 78 secure first-overtone classical Cepheids. Of these secure Cepheids, 420 are newly identified relative to the Shappee & Stanek catalog. The catalog also contains luminous candidates outside the classical Cepheid locus. We release the catalog and source-level two-band light curves for studies of Cepheid physics, stellar variability, and distance-scale applications.

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