Dissertations, Theses, and Capstone Projects

Date of Degree

6-2026

Document Type

Master's Thesis

Degree Name

Master of Science

Program

Astrophysics

Advisor

Ruth Angus

Advisor

Dax Feliz

Subject Categories

Physical Processes | Stars, Interstellar Medium and the Galaxy | The Sun and the Solar System

Keywords

stellar flares, cme, stars, exoplanets

Abstract

This thesis investigates whether archival TESS photometry and SDSS-V spectroscopy can be combined to identify coronal mass ejections (CMEs) from M dwarfs. Beginning from an initial sample of 625,155 SDSS-V targets, we developed a pipeline for cross-matching TESS photometric flare detections with contemporaneous SDSS-V spectroscopic visits, identifying 20 M dwarfs with overlapping coverage, and 3 visits (from 2 targets) obtained within 1 hour of a detected white-light flare. These two targets, and all corresponding spectra were analyzed in detail using local continuum normalization and Gaussian (single and double) MCMC line profile fitting of Hα and Hβ Balmer lines. For Target 1 (TIC 24056288/ SDSS ID 60965777) we confirm Hα and Hβ flare enhancement relative to quiescent visits, with no significant line asymmetry detected to indicate a potential CME. For Target 2 (TIC 233745344/ SDSS ID 69005520) we confirm Hα and Hβ line enhancement during the flare epoch, with an additional blue shifted Hβ component with a velocity offset of 160 km/s. At the spectral resolution of BOSS (R ∼ 2000, ∆v ≈ 150 km s−1), our sensitivity is limited to the highest-velocity CME signatures, consistent with the low detection rates reported in similar SDSS-based searches (Koller et al., 2021). We have also found this star to be a potential binary candidate so further follow up is needed to fully classify the detected asymmetry. Because of this uncertainty we find no robust detection of a CME. Nonetheless, this work establishes a scalable framework for future joint photometric-spectroscopic searches of stellar activity.

This work is embargoed and will be available for download on Wednesday, December 02, 2026

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