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Milli-Magnitude Time-Resolved Photometry with BEST

Karoff, Christoffer and Rauer, Heike and Erikson, Anders and Voss, Holger (2006) Milli-Magnitude Time-Resolved Photometry with BEST. Astronomical Society of the Pacific Conference Series (349), p. 261.

Full text not available from this repository.

Abstract

We present a comparative test of different photometry algorithms. The test has been made in order to optimize the number of stars for which light curves with milli-magnitude precision can be achieved in observations made by the Berlin Exoplanet Search Telescope (BEST), a small wide-angle telescope, located at Observatoire de Haute-Provence (OHP), France. The observations are part of an ongoing variability characterization of the target fields of the COROT space mission, therefore special attention is paid to overcome the problems introduced by crowding of the dense COROT fields. We also describe an algorithm for detecting variable stars in the data.

Item URL in elib:https://elib.dlr.de/43528/
Document Type:Article
Title:Milli-Magnitude Time-Resolved Photometry with BEST
Authors:
AuthorsInstitution or Email of AuthorsAuthors ORCID iD
Karoff, ChristofferUNSPECIFIEDUNSPECIFIED
Rauer, HeikeUNSPECIFIEDUNSPECIFIED
Erikson, AndersUNSPECIFIEDUNSPECIFIED
Voss, HolgerUNSPECIFIEDUNSPECIFIED
Date:2006
Journal or Publication Title:Astronomical Society of the Pacific Conference Series
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Page Range:p. 261
Status:Published
Keywords:BEST, Exoplanets, COROT
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - Vorhaben Extrasolare Planeten (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Extrasolar Planets and Atmospheres
Deposited By: Hedelt, Pascal
Deposited On:11 May 2006
Last Modified:14 Jan 2010 23:13

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