OGLE-2014-BLG-1186:gravitational microlensing providing evidence for a planet orbiting the foreground star or for a close binary source?

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OAIster

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Dominik , M , Bachelet , E , Bozza , V , Street , R A , Han , C , Hundertmark , M , Udalski , A , Bramich , D M , Alsubai , K A , Novati , S C , Ciceri , S , D'Ago , G , Jaimes , R F , Haugbolle , T , Hinse , T C , Horne , K , Jorgensen , U G , Juncher , D , Kains , N , Korhonen , H , Mancini , L , Menzies , J , Popovas , A , Rabus , M , Rahvar , S , Scarpetta , G , Schmidt , R , Skottfelt , J , Snodgrass , C , Southworth , J , Starkey , D , Steele , I A , Surdej , J , Tsapras , Y , Wambsganss , J , Wertz , O , Pietrukowicz , P , Szymanski , M K , Mroz , P , Skowron , J , Soszynski , I , Ulaczyk , K , Poleski , R , Wyrzykowski , L & Kozlowski , S 2019 , ' OGLE-2014-BLG-1186 : gravitational microlensing providing evidence for a planet orbiting the foreground star or for a close binary source? ' , Monthly Notices of the Royal Astronomical Society , vol. 484 , no. 4 , pp. 5608-5632 .

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application/pdf, English

Publication Type :

Electronic Resource

Accession number :

edsoai.on1322730819

Document Type :

Electronic Resource