Data from the TESScut

The folder contains three subfolders: flux, mag_after_lowess, and mag_no_lowess, which respectively represent measurement results expressed in flux values and magnitude values (including both detrended with lowess and non-detrended results). The same set of files appears in each subdirectory, containing results derived from distinct processing approaches. Which indicate the radii/pixel number of the selected aperture were 1.6/9, 2.1/13 and 3.0/19 pixels for sector 29 and 1.0/3, 1.6/5 and 2.1/8 pixels for sector 69, respectively. The background light curves of TIC198005083 (S4 and S30) and YZ Ret (S3 and S4). The light curves of TIC197934240 in sectors S3, S4, and S69. The light curves of YZ Ret from TESScut images.

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2025-04-25
DOI
https://doi.org/10.5281/zenodo.14553692
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
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article

Data from the TESScut

Zenodo (CERN European Organization for Nuclear Research)
Solar and Space Plasma Dynamics
article

Data from the TESScut

article en

Abstract

The folder contains three subfolders: flux, mag_after_lowess, and mag_no_lowess, which respectively represent measurement results expressed in flux values and magnitude values (including both detrended with lowess and non-detrended results). The same set of files appears in each subdirectory, containing results derived from distinct processing approaches. Which indicate the radii/pixel number of the selected aperture were 1.6/9, 2.1/13 and 3.0/19 pixels for sector 29 and 1.0/3, 1.6/5 and 2.1/8 pixels for sector 69, respectively. The background light curves of TIC198005083 (S4 and S30) and YZ Ret (S3 and S4). The light curves of TIC197934240 in sectors S3, S4, and S69. The light curves of YZ Ret from TESScut images.

Zenodo (CERN European Organization for Nuclear Research)
Openalex Percentile: Top 70%
Solar and Space Plasma Dynamics
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