Recent results by the MOA group on gravitational microlensing
P. Yock, I. Bond, N. Rattenbury, J. Skuljan, T. Sumi, FR. Abe, R. Dodd, J. Hearnshaw, M. Honda, J. Jugaku, P. Kilmartin, A. Marles, K. Masuda, Y. Matsubara, Y. Muraki, T. Nakamura, G. Nankivell, S. Noda, C. Noguchi, K. Ohnishi, M. Reid, To. Saito, H. Sato, M. Sekiguchi, D. Sullivan, M. Takeuti, Y. Watase, T. Yanagisawa
Abstract
Recent work by the MOA gravitational microlensing group is briefly described, including (i) the current observing strategy, (ii) use of a high-speed parallel computer for analysis of results by inverse ray shooting, (iii) analysis of the light curve of event OGLE-2000-BUL12 in terms of extra-solar planets, and (iv) the MOA alert system using difference imaging.
Create a lesson
Related papers
On binary pulsars and the force of gravity
Davor Palle
Tidal torques. A critical review of some techniques
Michael Efroimsky, James G. Williams
Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle Recombination
Rodrigo Fernández, Christopher Thompson
Asymptotically FRW black holes
J. T. Firouzjaee, Reza Mansouri
Reaction of Accretion Disks to Abrupt Mass Loss During Binary Black Hole Merger
Sean M. O'Neill, M. Coleman Miller, Tamara Bogdanovic et al.
A Gamma-Ray Burst/Pulsar for Cosmic-Ray Positrons with a Dark Matter-like Spectrum
Kunihito Ioka