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Robust detection of CID double stars in SDSS

Author(s): Pourbaix, D; Knapp, Gillian R; Gunn, James E.; Lupton, RH; Ivezic, Z; et al

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dc.contributor.authorPourbaix, D-
dc.contributor.authorKnapp, Gillian R-
dc.contributor.authorGunn, James E.-
dc.contributor.authorLupton, RH-
dc.contributor.authorIvezic, Z-
dc.contributor.authorSiopis, C-
dc.contributor.authorRigaux, M-
dc.contributor.authorRubbens, A-
dc.date.accessioned2022-01-25T14:58:03Z-
dc.date.available2022-01-25T14:58:03Z-
dc.date.issued2016-07en_US
dc.identifier.citationPourbaix, D, Knapp, GR, Gunn, JE, Lupton, RH, Ivezic, Z, Siopis, C, Rigaux, M, Rubbens, A. (2016). Robust detection of CID double stars in SDSS. ASTRONOMY & ASTROPHYSICS, 591 (10.1051/0004-6361/201628688en_US
dc.identifier.issn1432-0746-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr18k74w3q-
dc.description.abstractAims. The Sloan Digital Sky Survey (SDSS) offers a unique possibility of not only detecting colour induced displacement (CID) double stars but also confirming these detections. Methods. Successive cuts are applied to the SDSS data release (DR) 12 database to reduce the size of the sample under consideration. The resulting dataset is then screened with a criterion based on the distance and orientation of the photocentres in different photometric bands. Results. About 3200 distinct objects are classified as CID double stars, 40 of which are confirmed with at least a second detection. A consistency check further validates these detections.en_US
dc.language.isoen_USen_US
dc.relationhttps://ui.adsabs.harvard.edu/abs/2016A%26A...591A..96P/abstracten_US
dc.relation.ispartofASTRONOMY & ASTROPHYSICSen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleRobust detection of CID double stars in SDSSen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1051/0004-6361/201628688-
dc.date.eissued2016-06-21en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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