The Alpha Cygni (ACYG) variables are blue-white supergiants which display low-amplitude brightness variations of around 0.1 magnitude. The prototype Deneb shows quasi-periodic variations of around 12 days, interrupted by intervals of erratic variability, and occasionally large excursions in amplitude. To gain insight on the behavior of these variables, we examined 27-day light curves from the Transiting Exoplanet Survey Satellite (TESS) for 75 ACYG variables south of the ecliptic plane which are being revisited by TESS in 2025-2026. We use the web-based TESS Extractor app for screening TESS light curves. We identified ten stars with similarities to Deneb that may be good candidates for ground-based monitoring. We approximated the location of these stars on the Hertzsprung-Russell diagram, and find most lie below the Luminous Blue Variables, are cooler than the beta Cephei variables, and are hotter than the RV Tauri stars. We also compare light curves processed with several different pipelines available on the Mikulski Archive for Space Telescopes (MAST) and comment on their utility for ACYG stars.
Cite
@article{arxiv.2603.02421,
title = {Alpha Cygni Variables as Seen from the Transiting Exoplanet Survey Satellite},
author = {Joyce A. Guzik and Claire Whitley and Nova Moore and Madeline Marshall and Jason Jackiewicz},
journal= {arXiv preprint arXiv:2603.02421},
year = {2026}
}
Comments
17 pages, 14 figures, slightly updated version of paper submitted to Proceedings of the 114th Annual Meeting of the American Association of Variable Star Observers, Published January 2026, https://www.aavso.org/114