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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 6.

The scatter (median absolute deviation from the median (MAD)) of the individual channel completely processed (i.e., after performing magnitude fitting, EPD, and TFA steps) light curves vs. GAIA G magnitude, indicated by their corresponding channel color; i.e., B (blue), G1 (green), G2 (green), R (red)). These plots are for dither patterns D25 (left plots (a), (c), (e)) and D26 (right plots (b), (d), (f)), for each field G262(a, b), G111 (c, d), and G139 (e, f).

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