PyTranSpot: A tool for multiband light curve modeling of planetary transits and stellar spots

Ines G. Juvan; M. Lendl; P. E. Cubillos; L. Fossati; J. Tregloan-Reed; H. Lammer; E. W. Guenther; A. Hanslmeier

doi:10.1051/0004-6361/201731345

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Volume 610 (February 2018)

A&A, 610 (2018) A15

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Fig. A.5

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(O−C) residuals of the light curves SYNTH-4a to SYNTH-4d. All TLCs show the same transit event and occulted starspot around phase –0.002. The obtained photometric and spot parameters can be found in Tables B.2 and B.4.

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