Table 1.

Description of the parameters used to generate time series of CCFs with SOAP2. In each case, we give the number of spots (Nspot) and faculae (Nfac), as well as their corresponding stellar rotational phase ϕr and latitudes (Lat). The size of the active regions are set to 0.18 % (faculae) and 0.1 % (spot) with respect to the area of the visible hemisphere, in order to produce an RV signal of about 1 m s−1. The last column gives the number Npl of pure Doppler signals injected in the CCFs.

CaseNspotϕrLatNfacϕrLatNpl
[deg][deg]
(1)10.5000
(2)010.500
(3)20.0, 0.53020.25, 0.75300
(4)001
CaseNspotϕrLatNfacϕrLatNpl
[deg][deg]
(1)10.5000
(2)010.500
(3)20.0, 0.53020.25, 0.75300
(4)001
Table 1.

Description of the parameters used to generate time series of CCFs with SOAP2. In each case, we give the number of spots (Nspot) and faculae (Nfac), as well as their corresponding stellar rotational phase ϕr and latitudes (Lat). The size of the active regions are set to 0.18 % (faculae) and 0.1 % (spot) with respect to the area of the visible hemisphere, in order to produce an RV signal of about 1 m s−1. The last column gives the number Npl of pure Doppler signals injected in the CCFs.

CaseNspotϕrLatNfacϕrLatNpl
[deg][deg]
(1)10.5000
(2)010.500
(3)20.0, 0.53020.25, 0.75300
(4)001
CaseNspotϕrLatNfacϕrLatNpl
[deg][deg]
(1)10.5000
(2)010.500
(3)20.0, 0.53020.25, 0.75300
(4)001
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