High cadence near infrared timing observations of extrasolar planets - I. GJ 436b and XO-1b

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Table 1:

Observations and data reduction summary.
Target	Run	Date	Instrument	Window size (px)	DIT (s)	N. Frames	Filter	Apertures (px)	Inner annuli (px)
GJ 436b	A	May 17, 2007	SofI	$872\times132$	0.239	36 058	$K_{\rm S}$	23	35
XO-1b	A	April 27, 2007	SofI	$352\times152$	0.8	17 066	J	11	19
XO-1b	B	May 1, 2007	SofI	$892\times180$	0.8	20 100	J	8	20
XO-1b	C	May 1, 2007	ISAAC	$64\times544$	0.17-0.13^a	110 161	$K_{\rm S}$	7	10
XO-1b	D	May 5, 2007	ISAAC	$64\times544$	0.08	186 095	J+Block	21	21

^a The DIT (Detector Integration Time) was reduced during the observations to avoid reaching the non-linear limit of the detector in improving sky conditions.

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