Open AccessImproving the prospects for detecting extrasolar planets in gravitational microlensing events in 2002
Author(s) -
Bond I. A.,
Abe F.,
Dodd R. J.,
Hearnshaw J. B.,
Kilmartin P. M.,
Masuda K.,
Matsubara Y.,
Muraki Y.,
Noda S.,
Petterson O. K. L.,
Rattenbury N. J.,
Reid M.,
Saito To.,
Saito Y.,
Sako T.,
Skuljan J.,
Sullivan D. J.,
Sumi T.,
Wilkinson S.,
Yamada R.,
Yanagisawa T.,
Yock P. C. M.
Publication year - 2002
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2002.05374.x
Subject(s) - gravitational microlensing , physics , exoplanet , planet , astrophysics , astronomy , bulge , planetary system , gravitational lens , event (particle physics) , stars , galaxy , redshift
Gravitational microlensing events of high magnification have been shown to be promising targets for detecting extrasolar planets. However, only a few events of high magnification have been found using conventional survey techniques. Here we demonstrate that high‐magnification events can be readily found in microlensing surveys using a strategy that combines high‐frequency sampling of target fields with on‐line difference imaging analysis. We present 10 microlensing events with peak magnifications greater than 40 that were detected in real‐time towards the Galactic bulge during 2001 by the Microlensing Observations in Astrophysics (MOA) project. We show that Earth‐mass planets can be detected in future events such as these through intensive follow‐up observations around the event peaks. We report this result with urgency as a similar number of such events are expected in 2002.