HATS-13b and HATS-14b: two transiting hot Jupiters from the HATSouth survey

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Volume 580 (August 2015)

A&A, 580 (2015) A63

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Table 2

Summary of spectroscopy observations.

Telescope/instrument	UT date(s)	# Spec.	Res.	S/N range^a	γ _RV ^b	RV precision^c
			Δλ/λ/1000		(km s^-1)	(m s^-1)

HATS-13
ANU 2.3 m/WiFeS	2012 Apr. 10	1	3	90	···	···
ANU 2.3 m/WiFeS	2012 Apr. 11–12	2	7	30–40	25.0	1000
AAT 3.9 m/CYCLOPS	2012 May 5–11	4	70	10–20	25.8	190
Euler 1.2 m/Coralie	2012 Jun.–Nov.	9	60	12–17	25.8	100
MPG 2.2 m/FEROS	2012 May–Oct.	23	48	29–72	25.8	68
Subaru 8 m/HDS	2012 Sep. 19	3	60	17–32	···	···
Subaru 8 m/HDS+I₂	2012 Sep. 20–22	10	60	15–27	···	21
HATS-14
ANU 2.3 m/WiFeS	2012 Apr. 10	1	3	70	···	···
ANU 2.3 m/WiFeS	2012 Apr. 11–13	3	7	23–31	28.5	380
AAT 3.9 m/CYCLOPS	2012 May 5–11	5	70	15–25	29.9	110
Euler 1.2 m/Coralie	2012 Jun.–Nov.	14	60	9–16	30.2	37
MPG 2.2 m/FEROS	2012 May–2013 Jul.	17	48	25–68	30.2	12

Notes.

^(a)

S/N per resolution element near 5180 Å.

^(b)

For Coralie, FEROS and CYCLOPS this is the systemic RV from fitting an orbit to the observations in 3.3. For WiFeS it is the mean of the observations, and for the du Pont Echelle it is the measured RV of the single observation. We do not provide this quantity for instruments for which only relative RVs are measured, or for the lower resolution WiFeS observations which were only used to measure stellar atmospheric parameters.

^(c)

For High-precision RV observations included in the orbit determination this is the RV residuals from the best-fit orbit, for other instruments used for reconnaissance spectroscopy this is an estimate of the precision, or the measured standard deviation.

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