WASP-22 and WASP-26 photometry and velocities (Anderson+, 2011)

Details WASP-22 and WASP-26 photometry and velocities (Anderson+, 2011) WASP-22 and WASP-26 photometry and velocities (Anderson+, 2011)

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35349016a&link_type=abstract

VizieR On-line Data Catalog: J/A+A/534/A16. Originally published in: 2011A&A...534A..16A

Astronomy and Astrophysics

Astronomy

Binaries: Eclipsing, Planets, Radial Velocities, Photometry

Scientific paper

Using the HARPS spectrograph on the ESO 3.6-m telescope (La Silla, Chile), spectra of the planet host stars WASP-22 and WASP-26 were obtained through transits of their close-in planets, as well as across their orbits. The radial-velocity (RV) measurements extracted from the spectra are presented here. RVs were re-extracted from the six HARPS spectra of WASP-22 obtained by Maxted et al. (2010AJ....140.2007M) after removal of the instrumental blaze function (Triaud et al. 2010, Cat. J/A+A/524/A25) and are presented here.
Photometric transit observations of WASP-22 were obtained by the 0.6-m TRAPPIST and 1.2-m Euler telescopes (both at La Silla). A transit of WASP-26b was observed by the 0.35-m telescope at Oversky Observatory, La Palma. The Oversky data were originally made available at the Exoplanet Transit Database (http://var2.astro.cz/ETD/). The data are plotted in Figures 1 and 2.
(2 data files).

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