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20022009
most citedWater vapour in the atmosphere of a transiting extrasolar planet

379 citations · 454 across the 4 of their papers we have counts for

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10 papers · 1 filter

astro-ph200861 cited

Photometry using the Infrared Array Camera on the Spitzer Space Telescope

Joseph L. Hora, Sean Carey, Jason Surace +13

We present several corrections for point source photometry to be applied to data from the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. These corrections are necessa…

astro-ph20087 cited

Spitzer's mid-infrared view on an outer Galaxy Infrared Dark Cloud candidate toward NGC 7538

W. F. Frieswijk, M. Spaans, R. F. Shipman +3

Infrared Dark Clouds (IRDCs) represent the earliest observed stages of clustered star formation, characterized by large column densities of cold and dense molecular material observ…

astro-ph2007379 cited

Water vapour in the atmosphere of a transiting extrasolar planet

Giovanna Tinetti, Alfred Vidal-Madjar, Mao-Chang Liang +10

Water is predicted to be among, if not the most abundant molecular species after hydrogen in the atmospheres of close-in extrasolar giant planets (hot-Jupiters) Several attempts ha…

astro-ph2006

Ammonia in Infrared Dark Clouds

Thushara Pillai, Friedrich Wyrowski, Sean J. Carey +1

Infrared Dark Clouds appear to be the long sought population of cold and dense aggregations with the potential of harbouring the earliest stages of massive star formation. Up to no…

astro-ph2005

Absolute Calibration of the Infrared Array Camera on the Spitzer Space Telescope

William T. Reach, S. T. Megeath, Martin Cohen +10

The Infrared Array Camera (IRAC) on the Spitzer Space Telescope is absolutely calibrated by comparing photometry on a set of A stars near the north ecliptic pole to predictions bas…

astro-ph2005

Is the Cepheus E Outflow driven by a Class 0 Protostar?

A. Noriega-Crespo, A. Moro-Martin, S. Carey +4

New early release observations of the Cepheus E outflow and its embedded source, obtained with the Spitzer Space Telescope, are presented. We show the driving source is detected in…