Alcock, C.Allsman, R. A.Alves, David RAxelrod, T. S.Becker, A. C.Bennett, D. P.Chan, S.Cook, K. H.Drake, A.Freeman, K. C.Griest, K.Lehner, M. J.Marshall, S. L.Minniti, D.Peterson, B. A.Pratt, M. R.Quinn, P. J.Rodgers, A. W.Rorabeck, A.Sabine, S.Smillie, J.Stubbs, C. W.Sutherland, W.Tomaney, A.Turner, E.Vandehei, T.Welch, D. L.2018-09-142018-09-142013http://hdl.handle.net/1885/147535The MACHO Project was a collaboration between scientists at the Mt. Stromlo & Siding Spring Observatories, the Center for Particle Astrophysics at the Santa Barbara, San Diego, & Berkeley campuses of the University of California, and the Lawrence Livermore National Laboratory. Our primary aim was to test the hypothesis that a significant fraction of the dark matter in the halo of the Milky Way is made up of objects like brown dwarfs or planets: these objects have come to be known as MACHOs, for MAssive Compact Halo Objects. The signature of these objects is the occasional amplification of the light from extragalactic stars by the gravitational lens effect. The amplification can be large, but events are extremely rare: it was necessary to monitor photometrically several million stars for a period of 10 years in order to obtain a useful detection rate. For this purpose we built a two channel system that employed eight 2048*2048 CCDs, mounted on the 50 inch telescope at Mt. Stromlo. We have taken ~127,000 images with this system since June 1992. Analysis of a subset of these data has yielded databases containing light curves in two colors for 8 million stars in the LMC and 10 million in the bulge of the Milky Way.application/pdfen-AUhttps://creativecommons.org/licenses/by/4.0/High Energy AstrophysicsCosmic RaysPhysical SciencesAstronomical and Space SciencesOptical AstronomyLight CurvesDark Matterhttp://dx.doi.org/10.4225/13/5139255AB299610.4225/13/5139255AB2996The copyright to this collection is held under an Open Access license. The data for this collection can be accessed by anyone with an internet connection.