activity
20032008
most citedThe period-luminosity relation for type II Cepheids in globular clusters

94 citations · 139 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph2008

Science with UT's Dichroic-Mirror Camera (DMC), 15-band simultaneous imager

Hanindyo Kuncarayakti, Mamoru Doi, Hakim L. Malasan +20

We introduce the Dichroic-Mirror Camera (DMC), an instrument developed at the University of Tokyo which is capable of performing simultaneous imaging in fifteen bands. The main fea…

astro-ph200845 cited

Sequential star formation in a cometary globule (BRC37) of IC1396

Hisashi Ikeda, Koji Sugitani, Makoto Watanabe +9

We have carried out near-IR/optical observations to examine star formation toward a bright-rimmed cometary globule (BRC37) facing the exciting star(s) of an HII region (IC1396) con…

astro-ph200694 cited

The period-luminosity relation for type II Cepheids in globular clusters

Noriyuki Matsunaga, Hinako Fukushi, Yoshikazu Nakada +11

We report the result of our near-infrared observations (JHKs) for type II Cepheids (including possible RV Tau stars) in galactic globular clusters. We detected variations of 46 var…

astro-ph2005

Near Infrared Imaging Survey of Bok Globules: Density Structure

Ryo Kandori, Yasushi Nakajima, Motohide Tamura +11

On the basis of near-infrared imaging observations, we derived visual extinction (Av) distribution toward ten Bok globules through measurements of both the color excess (E_{H-K}) a…

astro-ph2005

A Distinct Structure Inside the Galactic Bar

Shogo Nishiyama, Tetsuya Nagata, Daisuke Baba +16

We present the result of a near-infrared (J H Ks) survey along the Galactic plane, -10.5deg < l < +10.5deg and b=+1.0deg, with the IRSF 1.4m telescope and the SIRIUS camera. Ks vs.…

astro-ph2003

Variable stars in the Magellanic Clouds: II. The data and infrared properties

Yoshifusa Ita, Toshihiko Tanabe, Noriyuki Matsunaga +10

The data of 8,852 and 2,927 variable stars detected by OGLE survey in the Large and Small Magellanic Clouds are presented. They are cross-identified with the SIRIUS JHK survey data…