期刊
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
卷 116, 期 817, 页码 266-277出版社
IOP PUBLISHING LTD
DOI: 10.1086/382735
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We discuss the system requirements for obtaining millimagnitude photometric precision over a wide field using small-aperture, short focal length telescope systems such as those being developed by a number of research groups to search for transiting extrasolar planets. We describe a Hungarian Automated Telescope ( HAT) system, which attempts to meet these requirements. The attainable precision of HAT has been significantly improved by a technique in which the telescope is made to execute small pointing steps during each exposure so as to broaden the effective point-spread function (PSF) of the system to a value more compatible with the pixel size of our CCD detector. Experiments during a preliminary survey ( spring 2003) of two star fields with the HAT-5 instrument allowed us to optimize the HAT photometric precision using this method of PSF broadening; in this way we have been able to achieve a precision as good as 2 mmag on brighter stars. We briefly describe development of a network of longitudinally spaced HAT telescopes (HATNet).
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