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Observational Limits on Terrestrial‐sized Inner Planets around the CM Draconis System Using the Photometric Transit Method with a Matched‐Filter Algorithm. / Doyle, Laurance; Deeg, Hans j.; Kozhevnikov, Valerij p. и др.
в: Astrophysical Journal, Том 535, № 1, 20.05.2000, стр. 338-349.

Результаты исследований: Вклад в журнал › Статья › Рецензирование

Harvard

Doyle, L, Deeg, HJ, Kozhevnikov, VP, Oetiker, B, Martin, EL, Blue, JE, Rottler, L, Stone, R, Ninkov, Z, Jenkins, J, Schneider, J, Dunham, EW, Doyle, MF & Paleologou, E 2000, 'Observational Limits on Terrestrial‐sized Inner Planets around the CM Draconis System Using the Photometric Transit Method with a Matched‐Filter Algorithm', Astrophysical Journal, Том. 535, № 1, стр. 338-349. https://doi.org/10.1086/308830

APA

Doyle, L., Deeg, H. J., Kozhevnikov, V. P., Oetiker, B., Martin, E. L., Blue, J. E., Rottler, L., Stone, R., Ninkov, Z., Jenkins, J., Schneider, J., Dunham, E. W., Doyle, M. F., & Paleologou, E. (2000). Observational Limits on Terrestrial‐sized Inner Planets around the CM Draconis System Using the Photometric Transit Method with a Matched‐Filter Algorithm. Astrophysical Journal, 535(1), 338-349. https://doi.org/10.1086/308830

Vancouver

Doyle L, Deeg HJ, Kozhevnikov VP, Oetiker B, Martin EL, Blue JE и др. Observational Limits on Terrestrial‐sized Inner Planets around the CM Draconis System Using the Photometric Transit Method with a Matched‐Filter Algorithm. Astrophysical Journal. 2000 май 20;535(1):338-349. doi: 10.1086/308830

Author

Doyle, Laurance ; Deeg, Hans j. ; Kozhevnikov, Valerij p. и др. / Observational Limits on Terrestrial‐sized Inner Planets around the CM Draconis System Using the Photometric Transit Method with a Matched‐Filter Algorithm. в: Astrophysical Journal. 2000 ; Том 535, № 1. стр. 338-349.

BibTeX

@article{154d9e9959e24f4fb31c92173522725f,
title = "Observational Limits on Terrestrial‐sized Inner Planets around the CM Draconis System Using the Photometric Transit Method with a Matched‐Filter Algorithm",
abstract = "A light curve of the eclipsing binary CM Draconis has been analyzed for the presence of transits of planets of size ≥ 2.5 Earth radii (RE), with periods of 60 days or less, and in coplanar orbits around the binary system. About 400 million model light curves, representing transits from planets with periods ranging from 7 to 60 days, have been matched/correlated against these data. This process we call the {"}transit detection algorithm{"} or TDA. The resulting {"}transit statistics{"} for each planet candidate allow the quantification of detection probabilities, and of false-alarm rates.",
author = "Laurance Doyle and Deeg, {Hans j.} and Kozhevnikov, {Valerij p.} and Brian Oetiker and Martin, {Eduardo l.} and Blue, {J. ellen} and Lee Rottler and Remington Stone and Zoran Ninkov and Jon Jenkins and Jean Schneider and Dunham, {Edward W.} and Doyle, {Moira F.} and Efthimious Paleologou",
year = "2000",
month = may,
day = "20",
doi = "10.1086/308830",
language = "English",
volume = "535",
pages = "338--349",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing (IOP)",
number = "1",

}

RIS

TY - JOUR

T1 - Observational Limits on Terrestrial‐sized Inner Planets around the CM Draconis System Using the Photometric Transit Method with a Matched‐Filter Algorithm

AU - Doyle, Laurance

AU - Deeg, Hans j.

AU - Kozhevnikov, Valerij p.

AU - Oetiker, Brian

AU - Martin, Eduardo l.

AU - Blue, J. ellen

AU - Rottler, Lee

AU - Stone, Remington

AU - Ninkov, Zoran

AU - Jenkins, Jon

AU - Schneider, Jean

AU - Dunham, Edward W.

AU - Doyle, Moira F.

AU - Paleologou, Efthimious

PY - 2000/5/20

Y1 - 2000/5/20

N2 - A light curve of the eclipsing binary CM Draconis has been analyzed for the presence of transits of planets of size ≥ 2.5 Earth radii (RE), with periods of 60 days or less, and in coplanar orbits around the binary system. About 400 million model light curves, representing transits from planets with periods ranging from 7 to 60 days, have been matched/correlated against these data. This process we call the "transit detection algorithm" or TDA. The resulting "transit statistics" for each planet candidate allow the quantification of detection probabilities, and of false-alarm rates.

AB - A light curve of the eclipsing binary CM Draconis has been analyzed for the presence of transits of planets of size ≥ 2.5 Earth radii (RE), with periods of 60 days or less, and in coplanar orbits around the binary system. About 400 million model light curves, representing transits from planets with periods ranging from 7 to 60 days, have been matched/correlated against these data. This process we call the "transit detection algorithm" or TDA. The resulting "transit statistics" for each planet candidate allow the quantification of detection probabilities, and of false-alarm rates.

UR - https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=tsmetrics&SrcApp=tsm_test&DestApp=WOS_CPL&DestLinkType=FullRecord&KeyUT=000087661900030

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=0034690381

U2 - 10.1086/308830

DO - 10.1086/308830

M3 - Article

VL - 535

SP - 338

EP - 349

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

ER -

ID: 42966394