Direct detection of a microlens in the Milky Way

Nature

Volumn 414, Issue 6864, 2001, Pages 617-619

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

^f AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^g LUCENT TECHNOLOGIES   (United States)

^h UNIVERSITY OF NOTRE DAME   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j UNIVERSITY OF CALIFORNIA   (United States)

^k PONTIFICIA UNIVERSIDAD CATÓLICA DE CHILE   (Chile)

^l UNIVERSITY OF WASHINGTON   (United States)

^m EUROPEAN SOUTHERN OBSERVATORY   (Germany)

ⁿ UNIVERSITY OF OXFORD   (United Kingdom)

^o MCMASTER UNIVERSITY   (Canada)

more..

Author keywords

[No Author keywords available]

Indexed keywords

GRAVITATION; LIGHT; LUMINOUS MATERIALS; MICROLENSES;

MILKY WAY;

ASTRONOMY;

EXTRATERRESTRIAL MATTER; SOLAR SYSTEM;

ARTICLE; ASTRONOMY; CAMERA; CLOUD; COSMOS; LENS; MASS; PRIORITY JOURNAL;

EID: 0035818996     PISSN: 00280836     EISSN: None     Source Type: Journal    
DOI: 10.1038/414617a     Document Type: Article

References (13)

1. Gravitational lensing by cold dark matter catastrophes
2. Deuterium and the baryonic density of the universe
3. The MACHO Project: Microlensing results from 5.7 years of Large Magellanic Cloud observations
4. The MACHO Project Hubble Space Telescope follow-up: Preliminary results on the location of the Large Magellanic Cloud microlensing source stars
5. The MACHO Project Large Magellanic Cloud microlensing results from the first two years and the nature of the Galactic dark halo
6. M dwarfs from Hubble Space Telescope star counts. III. The Groth Strip
7. The photometric performance and calibration of WFPC 2
8. First observation of parallax in a gravitational microlensing event
9. 6 M⊙
10. The late M dwarfs
11. Galactic globular clusters as a test for very-low-mass stellar models
12. Unresolved binaries and the stellar luminosity function
13. M dwarfs from Hubble Space Telescope star counts. IV