The Massive Compact Halo Object (MACHO) Project Data Archive
Short Name:
MACHO
Date:
23 Jul 2015 02:55:45
Publisher:
ivo://nci.org.au
Description:
The MACHO Project was a collaboration between scientists at the Mt. Stromlo and Siding Spring Observatories, the Center for Particle Astrophysics at the Santa Barbara, San Diego, and 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. The MACHO project data archive consists of approximately 127,000 two-colour images of fields collected between 1992 and 2003 covering the large and small Magellanic clouds and the galactic bulge and two-colour light-curves for approximately 18 million stars in the LMC and galactic bulge.
The WiggleZ Project Data Archive. The WiggleZ Dark Energy Survey is a survey of 240,000 emission-line galaxies measured with the AAOmega spectrograph of the 3.9-m Anglo-Australian Telescope (AAT). The aim of the survey is to measure the scale of baryon acoustic oscillations (BAO) imprinted on the spatial distribution of these galaxies. The survey will sample a volume of 1 Gpc3 over an area on the sky of 1000 square degrees with an average target density of 350 galaxies per square degree. The survey commenced in August 2006 and was completed in January 2011.
