TESS asteroseismology: new detections from main-sequence to subgiant stars
Monday
Abstract details
id
TESS asteroseismology: new detections from main-sequence to subgiant stars
Date Submitted
2021-04-29 10:39:00
Emily
Hatt
University of Birmingham
Science from TESS
Contributed
E. Hatt (University of Birmingham), M. Nielsen (University of Birmingham), W. Chaplin (University of Birmingham)
Asteroseismology has proven a powerful tool in constraining the physical properties of stars that oscillate like the Sun. The TESS satellite is providing new data on thousands of stars across different evolutionary phases, greatly expanding the potential for applying asteroseismology to characterize targets of interest. Utilizing a new pipeline developed to automate the detection of such stars, we present a catalogue of hundreds of new solar-like oscillators observed by TESS. This pipeline builds on the knowledge gained during the Kepler mission, applying it to a much broader range of targets, fully covering the sub-giant regime and extending down the main-sequence.
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