Table A17. Open in new tab Same as Table...

HJD-2 450 000.	M1	Mirror	2-Gaussian	Correlation
TIGRE
9336.908	−8.1	−10.6	−10.3	0.0
9437.820	−12.9	−15.3	−15.4	−5.0
9497.625	−10.1	−12.1	−12.2	−1.7
CARMENES
8696.617	−7.0	−8.8	−7.2	0.0
8712.486	−5.2	−6.0	−5.1	0.7
8756.464	−11.1	−14.3	−13.6	−4.7
8775.313	−13.8	−16.8	−16.1	−8.2
8792.342	−15.8	−19.0	−18.2	−11.0
9416.637	−17.2	−19.9	−20.0	−13.9
9438.586	−12.1	−14.6	−14.6	−7.9
9457.614	−9.2	−9.4	−9.0	−5.7
9477.461	−6.4	−6.8	−6.6	−2.8
9502.428	−12.3	−13.7	−13.3	−7.3

HJD-2 450 000.	M1	Mirror	2-Gaussian	Correlation
TIGRE
9336.908	−8.1	−10.6	−10.3	0.0
9437.820	−12.9	−15.3	−15.4	−5.0
9497.625	−10.1	−12.1	−12.2	−1.7
CARMENES
8696.617	−7.0	−8.8	−7.2	0.0
8712.486	−5.2	−6.0	−5.1	0.7
8756.464	−11.1	−14.3	−13.6	−4.7
8775.313	−13.8	−16.8	−16.1	−8.2
8792.342	−15.8	−19.0	−18.2	−11.0
9416.637	−17.2	−19.9	−20.0	−13.9
9438.586	−12.1	−14.6	−14.6	−7.9
9457.614	−9.2	−9.4	−9.0	−5.7
9477.461	−6.4	−6.8	−6.6	−2.8
9502.428	−12.3	−13.7	−13.3	−7.3

Table A17.

Same as Table A3 but for V2156 Cyg.

HJD-2 450 000.	M1	Mirror	2-Gaussian	Correlation
TIGRE
9336.908	−8.1	−10.6	−10.3	0.0
9437.820	−12.9	−15.3	−15.4	−5.0
9497.625	−10.1	−12.1	−12.2	−1.7
CARMENES
8696.617	−7.0	−8.8	−7.2	0.0
8712.486	−5.2	−6.0	−5.1	0.7
8756.464	−11.1	−14.3	−13.6	−4.7
8775.313	−13.8	−16.8	−16.1	−8.2
8792.342	−15.8	−19.0	−18.2	−11.0
9416.637	−17.2	−19.9	−20.0	−13.9
9438.586	−12.1	−14.6	−14.6	−7.9
9457.614	−9.2	−9.4	−9.0	−5.7
9477.461	−6.4	−6.8	−6.6	−2.8
9502.428	−12.3	−13.7	−13.3	−7.3

HJD-2 450 000.	M1	Mirror	2-Gaussian	Correlation
TIGRE
9336.908	−8.1	−10.6	−10.3	0.0
9437.820	−12.9	−15.3	−15.4	−5.0
9497.625	−10.1	−12.1	−12.2	−1.7
CARMENES
8696.617	−7.0	−8.8	−7.2	0.0
8712.486	−5.2	−6.0	−5.1	0.7
8756.464	−11.1	−14.3	−13.6	−4.7
8775.313	−13.8	−16.8	−16.1	−8.2
8792.342	−15.8	−19.0	−18.2	−11.0
9416.637	−17.2	−19.9	−20.0	−13.9
9438.586	−12.1	−14.6	−14.6	−7.9
9457.614	−9.2	−9.4	−9.0	−5.7
9477.461	−6.4	−6.8	−6.6	−2.8
9502.428	−12.3	−13.7	−13.3	−7.3

Note. The line was integrated from −475 to 475 km s⁻¹ for the moment method. Wings with normalized fluxes between 2.2 and 3.6 were used for the mirror method. The double Gaussians had center velocities ±a = ±175 km s⁻¹.

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