Looking for dark matter via gravitational microlensing: A report from the MACHO collaboration

Details Looking for dark matter via gravitational microlensing: A report from the MACHO collaboration Looking for dark matter via gravitational microlensing: A report from the MACHO collaboration

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aipc..342..106p&link_type=abstract

CAM-94 Physics meeting. AIP Conference Proceedings, Volume 342, pp. 106-112 (1995).

Physics

Dark Matter, Gravitational Lenses And Luminous Arcs

Scientific paper

There is convincing evidence that the mass of ordinary galaxies, like our own, is much greater than that measured in the form of stars, gas, and dust. If this dark matter is in the form of compact objects it can be detected via gravitational microlensing of background stars. The MACHO project is in its second year of a time resolved photometric survey of the Magellanic Clouds and galactic bulge to search for the rare microlensing signature of compact objects in the halo and disk of our galaxy. We are using a dedicated 1.3-m telescope at Mt. Stromlo Observatory and a dual focal plane CCD mosaic camera with a 0.5 square degree field to image up to 10 million stars per night simultaneously in two passbands. As of October 1994, 26,000 images have been taken with this system. A preliminary analysis of more than 8 million stars in the LMC for one year has yielded three stars which undergo time-symmetric achromatic photometric excursions consistent with gravitational microlensing. In a similar analysis of ~10 million stars in the galactic bulge we have also found more than 40 likely microlensing candidates, several of which reach peak amplifications of greater than ten. The relatively high rate toward the bulge is consistent with a ``maximal'' disk that accounts for most of the galactic mass interior to the solar radius or microlensing by a galactic bar.

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