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most citedHARP/ACSIS: A submillimetre spectral imaging system on the James Clerk Maxwell Telescope

231 citations · 2.1k across the 42 of their papers we have counts for

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astro-ph2007★ 172 cited

The James Clerk Maxwell Telescope Legacy Survey of Nearby Star-forming Regions in the Gould Belt

D. Ward-Thompson, J. Di Francesco, J. Hatchell +59

This paper describes a James Clerk Maxwell Telescope (JCMT) legacy survey that has been awarded roughly 500 hrs of observing time to be carried out from 2007 to 2009. In this surve…

astro-ph2007★ 12 cited

Observations of chemical differentiation in clumpy molecular clouds

J. V. Buckle, S. D. Rodgers, E. S. Wirström +4

We have extensively mapped a sample of dense molecular clouds (L1512, TMC-1C, L1262, Per 7, L1389, L1251E) in lines of HC3N, CH3OH, SO and C^{18}O. We demonstrate that a high degre…

astro-ph2006★ 27 cited

The JCMT Spectral Legacy Survey

R. Plume, G. A. Fuller, F. Helmich +30

Stars form in the densest, coldest, most quiescent regions of molecular clouds. Molecules provide the only probes which can reveal the dynamics, physics, chemistry and evolution of…

astro-ph2006★ 165 cited

JHK Observations of Faint Standard Stars in the Mauna Kea Near-Infrared Photometric System

S. K. Leggett, M. J. Currie, W. P. Varricatt +10

JHK photometry in the Mauna Kea Observatory (MKO) near-IR system is presented for 115 stars. Of these, 79 are UKIRT standards and 42 are LCO standards. The average brightness is 11…

astro-ph2004★ 210 cited

The host of GRB 030323 at z=3.372: a very high column density DLA system with a low metallicity

P. M. Vreeswijk, S. L. Ellison, C. Ledoux +29

We present photometry and spectroscopy of the afterglow of GRB 030323. VLT spectra of the afterglow show damped Lya (DLA) absorption and low- and high-ionization lines at a redshif…

astro-ph2003★ 19 cited

GRB 030227: the first multiwavelength afterglow of an INTEGRAL GRB

A. J. Castro-Tirado, J. Gorosabel, S. Guziy +39

We present multiwavelength observations of a gamma-ray burst detected by INTEGRAL (GRB 030227) between 5.3 hours and ~1.7 days after the event. Here we report the discovery of a di…