The macho project: Microlensing detection efficiency

Astrophysical Journal, Supplement Series

Volumn 136, Issue 2, 2001, Pages 439-462

  Alcock, C ^a,b   Allsman, R A ^c   Alves, D R ^d   Axelrod, T S ^c   Becker, A C ^e   Bennett, D P ^a,f   Cook, K H ^a,b   Drake, A J ^a,c   Freeman, K C ^c   Geha, M ^a   Griest, K ^b,g   Lehner, M J ^h   Marshall, S L ^a,b   Minniti, D ⁱ   Nelson, C A ^a,b   Peterson, B A ^c   Popowski, P ^a   Pratt, M R ^e   Quinn, P J ^j   Stubbs, C W ^b,c,e   Sutherland, W ^k   Tomaney, A B ^e   Vandehei, T ^b,g   Welch, D ^l   more..

^a LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^d AURA for the European Space Agency   (United States)

^e UNIVERSITY OF WASHINGTON   (United States)

^f UNIVERSITY OF NOTRE DAME   (United States)

^g UNIVERSITY OF CALIFORNIA   (United States)

^h UNIVERSITY OF SHEFFIELD   (United Kingdom)

ⁱ PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^j EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^k UNIVERSITY OF OXFORD   (United Kingdom)

^l MCMASTER UNIVERSITY   (Canada)

more..

Author keywords

Dark matter; Gravitational lensing; Methods: data analysis; Stars: low mass, brown dwarfs

Indexed keywords

EID: 18044365673     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/322529     Document Type: Article

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