| Crouzet et al. 2012 | spec | Hubble Space Telescope satellite | Near Infrared Camera and Multi-Object Spectrometer | 15 | CROUZET ET AL 2012 XO-1b was observed during 2 transit events, on 2008 February 10 and 2008 February 21. Each visit consists of 5 HST orbits. A total of 566 images were acquired, each with an exposure time of 40 s. The 1st orbit of each visit is rejected. In addition, the first 10 images of each orbit are affected by strong FWHM and temperature variations. This represents a small fraction of the data (18%), and these images are rejected. We thus construct the spectrum using the MCMC technique with a decorrelation of the instrumental parameters F0,x,y,α,w, and T, and x2. We construct a planetary spectrum from the 1st and 2nd visits independently, and for both visits analyzed simultaneously |
| Deming et al. 2013 | spec | Hubble Space Telescope satellite | Wide Field Camera 3 | 29 | DEMING ET AL 2013 Observations of HD 209458b and XO-1b used WFC3 with the G141 grism, providing wavelength coverage from1.0 - to 1.7μm in first order. Each star was observed during a single visit comprising 5 consecutive orbits. The observational sequence in each visit began with an undispersed image of the star using the F139M filter (centralwavelength of 1390 nm, and FWHM = 32 nm). The filter choice for this image is not crucial, because its purpose is merely to establish the position of the undispersed stellar image, used in wavelength calibration |
