activity
19962014
most citedMicrolensing optical depth towards the Galactic bulge from MOA observations during 2000 with Difference Image Analysis

231 citations · 328 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2014★ 28 cited

The First Very Long Baseline Interferometry Image of 44 GHz Methanol Maser with the KVN and VERA Array (KaVA)

Naoko Matsumoto, Tomoya Hirota, Koichiro Sugiyama +58

We have carried out the first very long baseline interferometry (VLBI) imaging of 44 GHz class I methanol maser (7_{0}-6_{1}A^{+}) associated with a millimeter core MM2 in a massiv…

astro-ph2005

Multi-epoch VERA Observations of H2O masers in OH 43.8-0.1

M. Honma, T. Bushimata, Y. K. Choi +33

We report on the multi-epoch observations of H2O maser emission in star forming region OH 43.8-0.1 carried out with VLBI Exploration of Radio Astrometry (VERA). The large-scale mas…

astro-ph2003★ 56 cited

First Fringe Detection with VERA's Dual-Beam System and its Phase Referencing Capability

M. Honma, T. Fujii, T. Hirota +25

We present the results of first dual-beam observations with VERA (VLBI Exploration of Radio Astrometry). The first dual-beam observations of a pair of H2O maser sources W49N and OH…

astro-ph2002★ 231 cited

Microlensing optical depth towards the Galactic bulge from MOA observations during 2000 with Difference Image Analysis

T. Sumi, F. Abe, I. A. Bond +27

We analyze the data of the gravitational microlensing survey carried out by by the MOA group during 2000 towards the Galactic Bulge (GB). Our observations are designed to detect ef…

astro-ph1996★ 13 cited

The Minimum Total Mass of MACHOs and Halo Models of the Galaxy

T. Nakamura, Y. Kan-ya, R. Nishi

If the density distribution ρ(r) of MACHOs is spherically symmetric with respect to the Galactic center, it is shown that the minimal total mass M_{min}^{ MACHO} of the MACHOs is 1…