Towards consistent mapping of distant worlds: secondary-eclipse scanning of the exoplanet HD 189733b

J. de Wit; M. Gillon; B.-O. Demory; S. Seager

doi:10.1051/0004-6361/201219060

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Volume 548 (December 2012)

A&A, 548 (2012) A128

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Table 1

AOR’s description.


AORKEY(⊕^a)	PI	Publication Ref.	Data sets^b (64x)	Exposure time [s]	Aperture [px]


16343552(O)	D. Charbonneau	Charbonneau et al. (2008)	1359	0.1	3.6
20673792(P)	D. Charbonneau	Knutson et al. (2007)	1319	0.4	4.8
22808832(O)
22809088(O)
22809344(O)
22810112(O)
24537600(O)
27603456(O)	E. Agol	Agol et al. (2010)	690	0.4	4.8


22807296(T)
22807552(T)
22807808(T)
24537856(T)
27603712(T)
27773440(T)	E. Agol	Agol et al. (2010)	690	0.4	4.8

Notes.

^(a)

AORKEY target: T, O or P respectively transit, occultation or phase curve.

^(b)

Present AOR are composed of data sets, each data set corresponds to 64 individual subarray images of 32 × 32 px.

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