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AutoWISP: Automated Processing of Wide-field Color Images

  • Authors: Angel E. Romero, Kaloyan Penev, S. Javad Jafarzadeh, Zoltan Csubry, Joel D. Hartman, Gáspár 'A. Bakos

Angel E. Romero et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 10.

The change in magnitude vs. phase plot of GG Dra (GDR3 1425033869225305728, Gaia G magnitude 8.6141). We determined its period to be 2.2695484 days from combining TESS and our data. (a.) Our light curve points (teal) are binned (circle teal points) and folded by the period. The corresponding TESS light curves (sectors 16, 23, 25, 50, 51, 52, 77, 78, 79, and 83, black points) are included. (b.) The binary system showed no color dependence (no obvious variance in red, blue, or green data points).

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