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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 7.

The scatter (median absolute deviation from the median (MAD)) of the combined channel completely processed (i.e., after performing magnitude fitting, EPD, and TFA steps) light curves vs. GAIA G magnitude (black points) for fields G262 (a), (b), G111 (c), (d), and G139 (e), (f) for dither patterns D25 (left) and D26 (right). For comparison, the red channel scatter is also shown (red points)

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