Masatoshi Ohishi

J-GLOBAL         Last updated: Jun 1, 2017 at 23:47
 
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Name
Masatoshi Ohishi
Affiliation
National Astronomical Observatory of Japan
Section
Astronomy Data Center
Job title
Associate Professor
Degree
PhD

Research Areas

 
 

Misc

 
Yutaka Komiya, Yuji Shirasaki, Masatoshi Ohishi, Yoshihiko Mizumoto
   Jun 2013
We present results of the cross-correlation analysis between active galactic
nuclei (AGNs) and galaxies at redshift 0.1-1. We obtain data of ~10,000 SDSS
AGNs in which their virial masses with a super-massive black hole (SMBH) were
estimated. The ...
Satoshi Eguchi, Wataru Kawasaki, Yuji Shirasaki, Yutaka Komiya, George Kosugi, Masatoshi Ohishi, Yoshihiko Mizumoto
   Nov 2012
ALMA is estimated to generate TB scale data during only one observation;
astronomers manage to identify which part of the data they are really
interested in. Now we have been developing new GUI software for this purpose
utilizing the VO interface:...
Inaki Ortiz, Jeff Lusted, Pat Dowler, Alexander Szalay, Yuji Shirasaki, Maria A. Nieto-Santisteban, Masatoshi Ohishi, William O'Mullane, Pedro Osuna, the VOQL-TEG Working Group, the VOQL Working Group
   Oct 2011
This document describes the Astronomical Data Query Language (ADQL). ADQL has
been developed based on SQL92. This document describes the subset of the SQL
grammar supported by ADQL. Special restrictions and extensions to SQL92 have
been defined in...
Yuji Shirasaki, Masahiro Tanaka, Masatoshi Ohishi, Yoshihiko Mizumoto, Naoki Yasuda, Tadafumi Takata
   Jul 2009
We present the result of projected cross correlation analysis of AGNs and
galaxies at redshifts from 0.3 to 3.0. The Japanese Virtual Observatory (JVO)
was used to obtain the Subaru Suprime-Cam images and UKIDSS catalog data around
AGNs. We invest...
Tomoya Hirota, Masatoshi Ohishi, Satoshi Yamamoto
Astrophys.J.699:585-602,2009      May 2009
We present results of a survey of CCS, HCTexN, and HCTexN toward 40
dark cloud cores to search for "Carbon-Chain--Producing Regions(CCPRs)", where
carbon-chain molecules are extremely abundant relative to NHTex, as in
L1495B, L1521B, L152...