The MACHO project Hubble Space Telescope follow-up: Preliminary results on the location of the large magellanic cloud microlensing source stars

Astrophysical Journal

Volumn 552, Issue 2 PART 1, 2001, Pages 582-590

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

^a LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c UNIVERSITY OF PENNSYLVANIA   (United States)

^d AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

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

^f LUCENT TECHNOLOGIES   (United States)

^g UNIVERSITY OF NOTRE DAME   (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j UNIVERSITY OF SHEFFIELD   (United Kingdom)

^k PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^l EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^m UNIVERSITY OF WASHINGTON   (United States)

ⁿ UNIVERSITY OF OXFORD   (United Kingdom)

more..

Author keywords

Dark matter; Galaxy: halo; Galaxy: structure; Gravitational lensing; Magellanic Clouds

Indexed keywords

EID: 0035837714     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/320554     Document Type: Article

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