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

Home

All issues

Volume 610 (February 2018)

A&A, 610 (2018) A15

Full HTML

Free Access

Fig. A.3

Open with DEXTER Download original image

(O−C) residuals of the synthetic light curves SYNTH-3a to SYNTH-3e. SYNTH-3e shows a starspot anomaly located close to the limb of the star around phase –0.005. The obtained photometric and spot parameters can be found in Tables B.1 and B.3.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.