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Statements

Subject Item
dbr:MACHO_Project
rdfs:label
MACHO Project
rdfs:comment
In astronomy, the MACHO Project was an observational search during 1992-1999 for dark matter around our Milky Way galaxy in the form of hypothetical Massive Compact Halo Objects (MACHOs), using the method of gravitational microlensing. It was one of three first-generation microlensing searches started in the early 1990s, the others being the independent EROS and OGLE projects. The MACHO project was carried out by a team of US and Australian astronomers; observations used the 1.27-metre (50-inch) telescope at the Mount Stromlo Observatory near Canberra, which was dedicated to the project full-time from 1992 until 1999. The project did not solve the dark matter problem, but placed important upper limits on the fraction of dark matter in MACHOs across a wide range of masses, and achieved seve
dct:subject
dbc:Astronomical_surveys dbc:Observational_astronomy
dbo:wikiPageID
43341809
dbo:wikiPageRevisionID
1117694660
dbo:wikiPageWikiLink
dbr:Microlensing dbr:Nancy_Grace_Roman_Space_Telescope dbr:Mount_Stromlo_Observatory dbc:Astronomical_surveys dbr:Gravitational_microlensing dbr:Large_Magellanic_Cloud dbr:Milky_Way dbr:Dark_matter dbr:OGLE dbr:Galactic_Bulge dbr:Gravitational_lensing dbr:Exoplanets dbr:2003_Canberra_bushfires dbr:Massive_Compact_Halo_Object dbc:Observational_astronomy dbr:KMTNet
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dbp:date
April 2021
dbp:reason
Placeholders in sentence should be defined
dbo:abstract
In astronomy, the MACHO Project was an observational search during 1992-1999 for dark matter around our Milky Way galaxy in the form of hypothetical Massive Compact Halo Objects (MACHOs), using the method of gravitational microlensing. It was one of three first-generation microlensing searches started in the early 1990s, the others being the independent EROS and OGLE projects. The MACHO project was carried out by a team of US and Australian astronomers; observations used the 1.27-metre (50-inch) telescope at the Mount Stromlo Observatory near Canberra, which was dedicated to the project full-time from 1992 until 1999. The project did not solve the dark matter problem, but placed important upper limits on the fraction of dark matter in MACHOs across a wide range of masses, and achieved several notable discoveries in the field of microlensing, and new results on several classes of variable stars.
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wikipedia-en:MACHO_Project?oldid=1117694660&ns=0
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9112
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wikipedia-en:MACHO_Project