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Physical Review Letters

Volumn 107, Issue 23, 2011, Pages

Microlensing of Kepler stars as a method of detecting primordial black hole dark matter

(4) Griest, Kim a Lehner, Matthew J b,c Cieplak, Agnieszka M a Jain, Bhuvnesh c

a UNIVERSITY OF CALIFORNIA (United States)

b INSTITUTE OF ASTRONOMY AND ASTROPHYSICS (Taiwan)

c UNIVERSITY OF PENNSYLVANIA (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ANGULAR SIZES; BLACK HOLES; CROSS SECTION; DARK MATTER; EXTRA SOLAR PLANETS; FINITE SOURCES; GRAVITATIONAL LENSING; KEPLER MISSION; LIGHT CURVES; MASS WINDOWS; MICRO-LENSING; NON-DETECTION; OPTICAL DEPTH; ORDERS OF MAGNITUDE; PHOTOMETRIC PRECISION;

NASA; PLANETS; STARS;

GRAVITATION;

EID: 82455174865 PISSN: 00319007 EISSN: 10797114 Source Type: Journal
DOI: 10.1103/PhysRevLett.107.231101 Document Type: Article

Times cited : (36)

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