Observational limits on terrestrial-sized inner planets around the CM Draconis system using the photometric transit method with a matched-filter algorithm

Astrophysical Journal

Volumn 535, Issue 1 PART 1, 2000, Pages 338-349

  Doyle, Laurance R ^a   Deeg, Hans J ^b,c   Kozhevnikov, Valerij P ^d   Oetiker, Brian ^e   Martín, Eduardo L ^b   Blue, J Ellen ^f   Rottler, Lee ^g   Stone, Remington P S ^h   Ninkov, Zoran ⁱ   Jenkins, Jon M ^j   Schneider, Jean ^k   Dunham, Edward W ^l   Doyle, Moira F ^m   Paleologou, Efthimious ⁿ  

^a Search for Extra terrestrial I I   (United States)

^b INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^c CENTRO DE ASTROBIOLOGÍA CSIC INTA   (Spain)

^d URAL FEDERAL UNIVERSITY   (Russian Federation)

^e UNIVERSITY OF NEW MEXICO   (United States)

^f SRI INTERNATIONAL   (United States)

^g University of California Santa Cruz   (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ ROCHESTER INSTITUTE OF TECHNOLOGY   (United States)

^j NASA AMES RESEARCH CENTER   (United States)

^k OBSERVATOIRE DE PARIS   (France)

^l LOWELL OBSERVATORY   (United States)

^m FIDM   (United States)

ⁿ UNIVERSITY OF CRETE   (Greece)

more..

Author keywords

Binaries : eclipsing; Methods : statistical; Planetary systems; Stars : Individual (CM Draconis); Techniques : photometric

Indexed keywords

EID: 0034690381     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/308830     Document Type: Article

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