J/ApJS/283/12       Solar-like oscillations using TESS 2           (Feng+, 2026)

Searching for Solar-like Oscillations Using TESS 2 minute Cadence in the Southern Ecliptic Hemisphere. Feng Y., Wu T., Xue H.-F., Li F., Niu J.-S. <Astrophys. J. Suppl. Ser. 283, 12 (2026)> =2026ApJS..283...12F 2026ApJS..283...12F (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable; Asteroseismology ; Effective temperatures; Abundances Keywords: Asteroseismology - Red giant stars - Light curves Abstract: The TESS space mission has generated an extensive collection of light curves, providing a valuable opportunity to search for solar-like oscillations. Numerous studies have utilized TESS observations to search for solar-like oscillations and achieved excellent results. However, the number of oscillators found by the previous works may be incomplete and significantly below the predicted count. Therefore, we employed a novel method to search for solar-like oscillations. In this work, we utilized TESS 2-minute cadence data to identify solar-like oscillators in the southern ecliptic hemisphere, detecting the presence of oscillations by identifying an excess power hump in the spectrum and combining visual inspection. As a result, we identified 10,548 stars exhibiting solar-like oscillations including 2972 that had not been reported in previous studies. The νmax and Δν of oscillators were determined using the fitting and autocorrelation, and the reliability of the Δ{nu measurements was further evaluated using the Fourier spectrum of the autocorrelation function. Based on this assessment, 4775 oscillators were classified as having reliable Δν, including 1920 that have Δν measured for the first time. Description: This catalog presents 10548 stars exhibiting solar-like oscillations identified from TESS 2-min cadence observations. The catalog is divided into two tables according to the reliability of the large frequency separation, Dnu. The file oscill1.dat contains 4775 stars with reliable Dnu measurements. The file oscill2.dat contains 5773 stars for which the Dnu measurements are not considered reliable. For each star, the catalog provides the TESS Input Catalog (TIC) identifier, basic stellar parameters, the frequency of maximum oscillation power (numax), the large frequency separation (Dnu), their uncertainties, and the number of TESS sectors used in the analysis. The effective temperature (Teff) and stellar radius (rad) are adopted from the TESS Input Catalog. The metallicity ([Fe/H]) and surface gravity (logg) are adopted from Gaia. The numax and Dnu parameters were determined in this work. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file oscill1.dat 80 4775 Stellar Global Oscillation Parameters, type 1 oscill2.dat 80 5773 Stellar Global Oscillation Parameters, type 2 -------------------------------------------------------------------------------- See also: IV/39 : TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021) Byte-by-byte Description of file: oscill1.dat oscill2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 I10 --- TIC TESS Input Catalog identifier 12- 16 I5 K Teff ? Effective temperature from the TIC 18- 24 F7.3 Rsun rad ? Stellar radius from the TIC 26- 32 F7.4 --- [Fe/H] ? Metallicity [Fe/H] from Gaia 34- 38 F5.3 [cm/s2] logg ? Surface gravity from Gaia 40- 45 F6.2 uHz numaxfit Frequency of maximum oscillation power from the fit 47- 52 F6.2 uHz e_numaxfit Uncertainty in numax_fit 54- 59 F6.2 uHz numax Frequency of maximum oscillation power 61- 66 F6.2 uHz e_numax Uncertainty in numax 68- 72 F5.2 uHz dnu Large frequency separation 74- 77 F4.2 uHz e_dnu Uncertainty in dnu 79- 80 I2 --- Nsectors Number of TESS sectors used -------------------------------------------------------------------------------- Acknowledgements: Yezheng Feng, 1569430671(at)qq.com License: CC-BY-4.0
(End) Patricia Vannier [CDS] 28-Aug-2026
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line