activity
20002010
most citedThe UKIRT Infrared Deep Sky Survey Early Data Release

221 citations · 980 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2010★ 33 cited

"Dark" GRB 080325 in a Dusty Massive Galaxy at z ~ 2

T. Hashimoto, K. Ohta, K. Aoki +30

We present optical and near infrared observations of GRB 080325 classified as a "Dark GRB". Near-infrared observations with Subaru/MOIRCS provided a clear detection of afterglow in…

astro-ph2006★ 54 cited

New members in the Upper Sco association from the UKIDSS Early Data Release

N. Lodieu, N. C. Hambly, R. F. Jameson

We present the results of a 9.3 square degree infrared (ZYJHK) survey in the Upper Scorpius association extracted from the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Cluster…

astro-ph2006★ 221 cited

The UKIRT Infrared Deep Sky Survey Early Data Release

S. Dye, S. J. Warren, N. C. Hambly +11

This paper defines the UKIRT Infrared Deep Sky Survey (UKIDSS) Early Data Release (EDR). UKIDSS is a set of five large near-infra-red surveys defined by Lawrence et al. (2006), bei…

astro-ph2004★ 45 cited

The proper motion of the isolated neutron star RX J1605.3+3249

C. Motch, K. Sekiguchi, F. Haberl +3

We obtained deep optical imaging of the thermally emitting X-ray bright and radio-quiet isolated neutron star RX J1605.3+3249 with the Subaru telescope in 1999 and 2003. Together w…

astro-ph2004★ 156 cited

Current Performance and On-Going Improvements of the 8.2 m Subaru Telescope

Masanori Iye, Hiroshi Karoji, Hiroyasu Ando +2

An overview of the current status of the 8.2 m Subaru Telescope constructed and operated at Mauna Kea, Hawaii, by the National Astronomical Observatory of Japan is presented. The b…

astro-ph2004★ 183 cited

Down-Sizing in Galaxy Formation at z~1 in the Subaru/XMM-Newton Deep Survey (SXDS)

Tadayuki Kodama

We use the deep wide-field optical imaging data of the Subaru/XMM-Newton Deep Survey (SXDS) to discuss the luminosity (mass) dependent galaxy colours down to z'=25.0 (5 x 10^9 h_{7…