First Results From Sleuth: The Palomar Planet Finder

dc.creatorO'Donovan, Francis T.
dc.creatorCharbonneau, David
dc.creatorKotredes, Lewis
dc.date2003-12-11
dc.date.accessioned2026-07-07T06:31:36Z
dc.date.available2026-07-07T06:31:36Z
dc.descriptionWe discuss preliminary results from our first search campaign for transiting planets performed using Sleuth, an automated 10 cm telescope with a 6 degree square field of view. We monitored a field in Hercules for 40 clear nights between UT 2003 May 10 and July 01, and obtained an rms precision (per 15-min average) over the entire data set of better than 1% on the brightest 2026 stars, and better than 1.5% on the brightest 3865 stars. We identified no strong candidates in the Hercules field. We conducted a blind test of our ability to recover transiting systems by injecting signals into our data and measuring the recovery rate as a function of transit depth and orbital period. About 85% of transit signals with a depth of 0.02 mag were recovered. However, only 50% of transit signals with a depth of 0.01 mag were recovered. We expect that the number of stars for which we can search for transiting planets will increase substantially for our current field in Andromeda, due to the lower Galactic latitude of the field.
dc.description4 pages, 4 figures, to appear in AIP Conf Proc: The Search for Other Worlds, eds. S. S. Holt & D. Deming
dc.identifierhttps://arxiv.org/abs/astro-ph/0312289
dc.identifierhttp://arxiv.org/abs/astro-ph/0312289
dc.identifierAIP Conf. Proc. 713, 169 (2004)
dc.identifierdoi:10.1063/1.1774518
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/98654
dc.subjectAstrophysics
dc.titleFirst Results From Sleuth: The Palomar Planet Finder
dc.typetext

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