Search for Low-Mass Exoplanets by Gravitational Microlensing at High Magnification
- 27 August 2004
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 305 (5688) , 1264-1266
- https://doi.org/10.1126/science.1100714
Abstract
Observations of the gravitational microlensing event MOA 2003-BLG-32/OGLE 2003-BLG-219 are presented, for which the peak magnification was over 500, the highest yet reported. Continuous observations around the peak enabled a sensitive search for planets orbiting the lens star. No planets were detected. Planets 1.3 times heavier than Earth were excluded from more than 50% of the projected annular region from approximately 2.3 to 3.6 astronomical units surrounding the lens star, Uranus-mass planets were excluded from 0.9 to 8.7 astronomical units, and planets 1.3 times heavier than Saturn were excluded from 0.2 to 60 astronomical units. These are the largest regions of sensitivity yet achieved in searches for extrasolar planets orbiting any star.Keywords
All Related Versions
This publication has 24 references indexed in Scilit:
- OGLE 2003-BLG-235/MOA 2003-BLG-53: A Planetary Microlensing EventThe Astrophysical Journal, 2004
- The Search for Pale Blue DotsScience, 2004
- Microlensing Constraints on the Frequency of Jupiter‐Mass Companions: Analysis of 5 Years of PLANET PhotometryThe Astrophysical Journal, 2002
- On Planetary Companions to the MACHO 98‐BLG‐35 Microlens StarThe Astrophysical Journal, 2000
- The Initial Mass Function of the Galactic Bulge down to ∼0.15M⊙The Astrophysical Journal, 2000
- The Use of High‐Magnification Microlensing Events in Discovering Extrasolar PlanetsThe Astrophysical Journal, 1998
- The Luminosity Function and Initial Mass Function in the Galactic BulgeThe Astronomical Journal, 1998
- Detecting Earth‐Mass Planets with Gravitational MicrolensingThe Astrophysical Journal, 1996
- Discovering planetary systems through gravitational microlensesThe Astrophysical Journal, 1992
- Gravitational microlensing by double stars and planetary systemsThe Astrophysical Journal, 1991