Gaia eclipsing binary and multiple systems - Two-Gaussian models applied to OGLE-III eclipsing binary light curves in the Large Magellanic Cloud

N. Mowlavi; I. Lecoeur-Taïbi; B. Holl; L. Rimoldini; F. Barblan; A. Prša; A. Kochoska; M. Süveges; L. Eyer; K. Nienartowicz; G. Jevardat; J. Charnas; L. Guy; M. Audard

doi:10.1051/0004-6361/201730613

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Volume 606 (October 2017)

A&A, 606 (2017) A92

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Fig. 21

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Examples of folded light curves in region C of the versus that have large intrinsic scatter in their residuals. The colors of the models are the same as in Fig. 6. Their positions in the versus diagram are labeled in Fig. 19.

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