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The POINT-AGAPE Microlensing Survey: First Constraint on MACHOs towards M31
Paulin-Henriksson S., Calchi-Novati S.
XXXIXth Rencontres de Moriond "Exploring the Universe", La Thuile : Italie (2004) - http://hal.in2p3.fr/in2p3-00022282
Physique/Astrophysique/Cosmologie et astrophysique extra-galactique
The POINT-AGAPE Microlensing Survey: First Constraint on MACHOs towards M31
S. Paulin-Henriksson1, S. Calchi-Novati
1 :  PCC - Physique Corpusculaire et Cosmologie - Collège de France
CNRS : UMR7553 – IN2P3 – Université Paris VII - Paris Diderot
11, place Marcelin Berthelot - 75231 Paris Cedex 05
France
To reveal the galactic dark matter in the form of MACHOs ("Massive Astrophysical Compact Halo Objects"), the POINT-AGAPE collaboration is carrying out a search for gravitational microlensing towards M31. A clear microlensing signal is detected. The high-threshold analysis of 3-year data leads to 7 bright and short microlensing candidates. The preliminary estimation of the detection efficiency implies that less than 25% (60%) of standard halos can be composed of objects with masses between 10^{-4} and 10^{-1} (10^{-1} and 1) solar mass at the 95% C.L. This result is compatible with previous microlensing results towards the Magellanic Clouds and gives the first constraints on MACHOs for a distant spiral galaxy.
AGAPE

Communications sans actes
2004

XXXIXth Rencontres de Moriond "Exploring the Universe"
La Thuile
Italie
28/03/2004
04/04/2004

PCC 04 46/Conf
The POINT-AGAPE Collaboration

Lien vers le texte intégral : 
http://fr.arXiv.org/abs/astro-ph/0408204