High-Precision Multi-Period Analysis of the Ellipsoidal Variable Candidate TIC~470127886 from TESS Photometry
Roo Weerasinghe

TL;DR
This paper presents a detailed, high-precision photometric analysis of TIC 470127886, revealing complex multi-periodic variability consistent with an ellipsoidal binary, using extensive TESS data over nearly three years.
Contribution
It provides the first detailed characterization of TIC 470127886, identifying multiple significant periods and modeling its variability as an ellipsoidal binary candidate with high confidence.
Findings
Identified three significant periods at approximately 5.55, 5.80, and 8.87 days.
Confirmed the variability is consistent with tidal distortion in a close binary system.
Validated the signal's authenticity and ruled out contamination from nearby stars.
Abstract
We present the first detailed photometric characterization of TIC 470127886, a previously unstudied multi-periodic variable star discovered in TESS photometry. Analysis of 145,374 high-cadence observations spanning 696 days (944-day baseline, 2023 January-2024 October) across 10 sectors (60, 59, 58, 53, 52, 73, 86, 79, 78, 85) reveals complex periodic variability with a primary period of 5.544527 +/- 0.004307 days and false alarm probability 1.47 x 10^-87. Lomb-Scargle analysis identifies three significant periods at 5.545, 5.801, and 8.874 days with amplitudes of 15,702, 12,772, and 12,670 ppm. The phase-folded light curve shows smooth, sinusoidal morphology consistent with ellipsoidal variation from tidal distortion in a close binary, with no eclipse features. A three-component sinusoidal model, appropriate for ellipsoidal variables, provides excellent fit quality. Validation tests…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Solar and Space Plasma Dynamics
