Analysis of combined radial velocities and activity of BD+20 1790: evidence supporting the existence of a planetary companion

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Volume 576 (April 2015)

A&A, 576 (2015) A66

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Table 2

Observing runs.

Date	Telescope	Instrument	CCD chip	Spect. range	Orders	Dispersion	FWHM	S/N
			#	(Å)		(Å/pix)	(Å)

31/01/2008	2.2m^a	FOCES	2048 × 2048 15 μm LORAL#11i	3830–10850	96	0.03–0.07	0.09–0.26	80
31/03-2/04/2010	TNG^b	SARG	2148 × 4200 13.5 μm EEV	5480–10120	51	0.08–0.14	0.16–0.32	140
9-11/02/2009	NOT^c	FIES	2000 × 2000 15 μm EEV42-40	3620–7360	79	0.02–0.04	0.05–0.11	70
22-25/12/2010	Mercator^d	HERMES	2048 × 4608 24 μm E2V42-90	3770–9000	58	0.016–0.13	0.08–0.35	120
27-31/12/2012	TNG^b	HARPS-N	4k4 24 μm E2V	3830–6930	68	0.03–0.06	0.03–0.06	30
22-25/02/2013	TNG^b	HARPS-N	4k4 24 μm E2V	3830–6930	68	0.03–0.06	0.03–0.06	30
21-24/01/2014	TNG^b	HARPS-N	4k4 24 μm E2V	3830–6930	68	0.03–0.06	0.03–0.06	30
18/05/2014	TNG^b	HARPS-N	4k4 24 μm E2V	3830–6930	68	0.03–0.06	0.03–0.06	30

Notes.

^(a)

2.2 m telescope at the German Spanish Astronomical Observatory (CAHA) (Almería, Spain).

^(b)

3.58 m Telescopio Nazionale Galileo (TNG) at Observatorio del Roque de los Muchachos (La Palma, Spain).

^(c)

2.5 m Nordic Optical Telescope (NOT) at Observatorio del Roque de los Muchachos (La Palma, Spain).

^(d)

1.2 m Mercator Telescope at Observatorio del Roque de los Muchachos (La Palma, Spain).

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