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The Vulcan Photometer: A Dedicated Photometer for Extrasolar Planet Searches

2001; Institute of Physics; Volume: 113; Issue: 782 Linguagem: Inglês

10.1086/319537

1538-3873

W. J. Borucki, Douglas A. Caldwell, David Koch, L. D. Webster, Jon M. Jenkins, Zoran Ninkov, Robert L. Showen,

Astronomy and Astrophysical Research

A small CCD photometer dedicated to the detection of extrasolar planets has been developed and put into operation at Mount Hamilton, California. It simultaneously monitors 6000 stars brighter than 13th magnitude in its 49 deg2 field of view. Observations are conducted all night every clear night of the year. A single field is monitored at a cadence of eight images per hour for a period of about 3 months. When the data are folded for the purpose of discovering low‐amplitude transits, transit amplitudes of 1% are readily detected. This precision is sufficient to find Jovian‐size planets orbiting solar‐like stars, which have signal amplitudes from 1% to 2% depending on the inflation of the planet's atmosphere and the size of the star. An investigation of possible noise sources indicates that neither star field crowding, scintillation noise, nor photon shot noise are the major noise sources for stars brighter than visual magnitude 11.6.