activity
20002008
most citedEvidence for a companion to BM Gem, a silicate carbon star

16 citations · 33 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph200816 cited

Evidence for a companion to BM Gem, a silicate carbon star

Hideyuki Izumiura, Kunio Noguchi, Wako Aoki +12

Balmer and Paschen continuum emission as well as Balmer series lines of P Cygni-type profile from H_gamma through H_23 are revealed in the violet spectra of BM Gem, a carbon star a…

astro-ph200714 cited

Observation of the first gravitational microlensing event in a sparse stellar field : the Tago event

A. Fukui, F. Abe, K. Ayani +17

We report the observation of the first gravitational microlensing event in a sparse stellar field, involving the brightest (V=11.4 mag) andclosest (~ 1 kpc) source star to date. Th…

astro-ph20061 cited

Constructing the Subaru Advanced Data and Analysis Service on VO

Yuji Shirasaki, Masahiro Tanaka, Satoshi Honda +10

We present our activity on making the Subaru Data Archive accessible through the Japanese Virtual Observatory (JVO) system. There are a lot of demand to use the archived Subaru dat…

astro-ph20062 cited

Japanese Virtual Observatory (JVO) as an advanced astronomical research enviroment

Y. Shirasaki, M. Tanaka, S. Kawanomoto +10

We present the design and implementation of the Japanese Virtual Observatory (JVO) system. JVO is a portal site to various kinds of astronomical resources distributed all over the…

astro-ph2004

A low upper-limit on the lithium isotope ratio in HD140283

Wako Aoki, Susumu Inoue, Satoshi Kawanomoto +4

We have obtained a high-S/N (900-1100), high-resolving-power (R=95000) spectrum of the metal-poor subgiant HD 140283 in an effort to measure its 6Li/7Li isotope ratio. From a 1-D a…

astro-ph2004

Spectroscopic Studies of Extremely Metal-Poor Stars with Subaru/HDS:I. Observational Data

S. Honda, W. Aoki, H. Ando +14

We have obtained high-resolution (R 50,000 or 90,000), high-quality (S/N $\ga$ 100) spectra of 22 very metal-poor stars ([Fe/H] $\la$ -2.5) with the High Dispersion Spectr…