Evidence of a massive planet candidate orbiting the young active K5V star BD+20 1790

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Volume 512 (March-April 2010)

A&A, 512 (2010) A45

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Table 2:

Observing runs.
Date	Telescope	Instrument	CCD chip	Spect. range	Orders	Dispersion	FWHM^c	N. Obs.
			#	(Å)		(Å/pix)	(Å)
29/03-6/04 2004	2.2 m^a	FOCES	2048 $\times$ 2048 24 $\mu$ m Site $\char93$ 1d	3720-10 850	100	0.04-0.13	0.08-0.35	19
21-22/11/2004	TNG ^b	SARG	2048 $\times$ 4096 13.5 $\mu$ m EEV	4620-7920	52	0.07-0.11	0.07-0.17	43
15/04/2006	TNG ^b	SARG	2048 $\times$ 4096 13.5 $\mu$ m EEV	4620-7920	52	0.07-0.11	0.07-0.17	14
2-5/10/2007	2.2 m^a	FOCES	2048 $\times$ 2048 24 $\mu$ m Site $\char93$ 1d	3720-10 850	100	0.04-0.13	0.08-0.35	10
12-13/12/2008	2.2 m^a	FOCES	2048 $\times$ 2048 15 $\mu$ m LORAL $\char93$ 11i	3830-10 850	96	0.03-0.07	0.09-0.26	2
19-21/12/2008	2.2 m^a	FOCES	2048 $\times$ 2048 24 $\mu$ m Site $\char93$ 1d	3720-10 850	100	0.04-0.13	0.08-0.35	3

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) The spectral resolution is determined as the FWHM at the arc comparison lines ranges.

Source LaTeX | All tables | In the text

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