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 1

Summary of photometric observations.

Instrument/field^a	UT date(s)	# Images	Cadence^b	Filter	Precision^c
			(s)		(mmag)

HATS-13
HS-2/G582	2009 Nov.–2010 Sep.	2486	288	r	12.6
HS-4/G582	2009 Sep.–2010 Sep.	8565	288	r	12.2
HS-6/G582	2010 Apr.–2010 Sep.	356	265	r	13.1
CTIO 0.9 m^d	2012 Aug. 26	68	237	z	2.9
MPG 2.2 m/GROND^d	2012 Oct. 17	82	87	g	1.4
MPG 2.2 m/GROND^d	2012 Oct. 17	83	87	r	1.2
MPG 2.2 m/GROND^d	2012 Oct. 17	82	87	i	1.7
MPG 2.2 m/GROND^d	2012 Oct. 17	82	87	z	1.6
PEST	2013 May 3	99	130	R	4.7
PEST	2013 Jun. 30	189	130	R	4.7
HATS-14
HS-2/G582	2009 Nov.–2010 Sep.	4866	284	r	11.5
HS-4/G582	2009 Sep.–2010 Sep.	8889	288	r	12.6
HS-6/G582	2010 Aug.–2010 Sep.	200	290	r	11.6
PEST	2013 Jun. 06	131	131	R	4.8
MPG 2.2 m/GROND^d	2013 Jun. 12	114	192	g	1.6
MPG 2.2 m/GROND^d	2013 Jun. 12	114	192	r	1.8
MPG 2.2 m/GROND^d	2013 Jun. 12	114	192	i	2.6
MPG 2.2 m/GROND^d	2013 Jun. 12	114	192	z	2.0

Notes.

^(a)

For HATSouth data we list the HATSouth unit and field name from which the observations are taken. HS-1 and -2 are located at Las Campanas Observatory in Chile, HS-3 and -4 are located at the HESS site in Namibia, and HS-5 and -6 are located at Siding Spring Observatory in Australia. Each field corresponds to one of 838 fixed pointings used to cover the full 4π celestial sphere. All data from a given HATSouth field are reduced together, while detrending through External Parameter Decorrelation (EPD) is done independently for each unique field+unit combination.

^(b)

The median time between consecutive images rounded to the nearest second. Due to weather, the day-night cycle, guiding and focus corrections, and other factors, the cadence is only approximately uniform over short timescales.

^(c)

The root mean square of the residuals from the best-fit model.

^(d)

The telescope-defocussing technique (Southworth et al. 2009) was used for this transit observation.

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