Distinguishing the albedo of exoplanets from stellar activity

L. M. Serrano; S. C. C. Barros; M. Oshagh; N. C. Santos; J. P. Faria; O. Demangeon; S. G. Sousa; M. Lendl

doi:10.1051/0004-6361/201731206

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Volume 611 (March 2018)

A&A, 611 (2018) A8

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Table 4

Spot properties used to generate the activity patterns of the blind tests with SOAP (Oshagh et al. 2013b).

Pattern	Spot	Longitude	Brightness	Size (R_*)
	1	0^°	0.50	0.080
	2	55^°	0.48	0.075
a	3	120^°	0.52	0.081
	4	174^°	0.48	0.079
	5	227^°	0.50	0.083

	6	290^°	0.49	0.076
	1	0^°	0.50	0.040
b	2	20^°	0.48	0.045
	3	35^°	0.52	0.041
	4	121^°	0.48	0.049

	1	0^°	0.50	0.02
c	2	34^°	0.48	0.025

Notes. The pattern labeled a has been adopted for tests 1–3, the b pattern for tests 4–6, and thec pattern for the last three tests. This information was unknown by the person that performed the analysis.

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