The POINT-AGAPE survey: 4 High signal-to-noise microlensing candidates detected towards M 31

Astronomy and Astrophysics

Volumn 405, Issue 1, 2003, Pages 15-21

  Paulin Henriksson, S ^a   Baillon, P ^b   Bouquet, A ^a   Carr, B J ^c   Creze M ^a,d   Evans, N W ^e,f   Giraud Heraud Y ^a   Gould, A ^a,g   Hewett, P ^a,f   Kaplan, J ^a   Kerins, E ^a,h   Le Du, Y ^a,e   Melchior, A L ⁱ   Smartt, S J ^f   Valls Gabaud, D ^j  

^a l'alimentation et l'Environnement   (France)

^b CERN   (Switzerland)

^c QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^d UNIVERSITÉ BRETAGNE SUD   (France)

^e UNIVERSITY OF OXFORD   (United Kingdom)

^f UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^g OHIO STATE UNIVERSITY   (United States)

^h LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

ⁱ OBSERVATOIRE DE PARIS   (France)

^j OBSERVATOIRE MIDI PYRÉNÉES   (France)

more..

Author keywords

Dark matter; Galaxies: halo; Galaxies: individual: M 31; Gravitational lensing

Indexed keywords

GALAXIES; MICROLENSES; SIGNAL TO NOISE RATIO;

UNRESOLVED MICROLENSING;

ASTROPHYSICS;

EID: 0037561231     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030519     Document Type: Review

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