The applicability of the astrometric method for determining the physical parameters of gravitational microlenses
Open Access
- 16 April 1999
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 304 (4) , 845-850
- https://doi.org/10.1046/j.1365-8711.1999.02368.x
Abstract
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This publication has 14 references indexed in Scilit:
- Astrometric Observation of MACHO Gravitational MicrolensingThe Astrophysical Journal, 1998
- The MACHO Project Large Magellanic Cloud Microlensing Results from the First Two Years and the Nature of the Galactic Dark HaloThe Astrophysical Journal, 1997
- The Effects of Amplification Bias in Gravitational Microlensing ExperimentsThe Astrophysical Journal, 1997
- The MACHO Project: 45 Candidate Microlensing Events from the First Year Galactic Bulge DataThe Astrophysical Journal, 1997
- Space Interferometry Mission: taking the measure of the universePublished by SPIE-Intl Soc Optical Eng ,1997
- The Mass Spectrum of MACHOs from Parallax MeasurementsThe Astrophysical Journal, 1995
- Proper motions of MACHOsThe Astrophysical Journal, 1994
- Galactic structure from the spacelab infrared telescope. III - A dynamical model for the Milky Way bulgeThe Astrophysical Journal, 1992
- Star Counts and Galactic StructureAnnual Review of Astronomy and Astrophysics, 1986
- The galactic spheroidThe Astrophysical Journal, 1983