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20032009
most citedThe Arecibo Galaxy Environment Survey: Precursor Observations of the NGC 628 group

80 citations · 299 across the 6 of their papers we have counts for

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astro-ph200761 cited

Sub-millimeter Observations of Giant Molecular Clouds in the Large Magellanic Cloud: Temperature and Density as Determined from J=3-2 and J=1-0 transitions of CO

T. Minamidani, N. Mizuno, Y. Mizuno +26

We have carried out sub-mm 12CO(J=3-2) observations of 6 giant molecular clouds (GMCs) in the Large Magellanic Cloud (LMC) with the ASTE 10m sub-mm telescope at a spatial resolutio…

astro-ph2007

The ALFA Zone of Avoidance Survey: Results from the Precursor Observations

C. M. Springob, P. A. Henning, B. Catinella +11

The Arecibo L-band Feed Array Zone of Avoidance Survey (ALFA ZOA) will map 1350-1800 square degrees at low Galactic latitude, providing HI spectra for galaxies in regions of the sk…

astro-ph200725 cited

The Origin of Large-scale HI structures in the Magellanic Bridge

E. Muller, K. Bekki

We investigate the formation of a number of key large-scale HI features in the ISM of the Magellanic Bridge using dissipationless numerical simulation techniques. This study compri…

astro-ph200666 cited

First results from the Arecibo Galactic HI Survey: the disk/halo interface region in the outer Galaxy

Snezana Stanimirovic, Mary Putman, Carl Heiles +11

The consortium for Galactic studies with the Arecibo L-band Feed Array (ALFA) is conducting a neutral hydrogen (HI) survey of the whole Arecibo sky (declination range from -1 to 38…

astro-ph200680 cited

The Arecibo Galaxy Environment Survey: Precursor Observations of the NGC 628 group

R. Auld, R. F. Minchin, J. I. Davies +25

The Arecibo Galaxy Environment Survey (AGES) is one of several HI surveys utilising the new Arecibo L-band Feed Array (ALFA) fitted to the 305m radio telescope at Arecibo. The surv…

astro-ph2005

Stellar mass loss and the Intra-Cluster Medium in Galactic globular clusters: a deep radio survey for HI and OH

Jacco Th. van Loon, Snezana Stanimirovic, A. Evans +1

We present the results of a survey, the deepest to date, for HI emission at 21 cm and OH emission at 18 cm (lines at 1612, 1665, 1667 and 1720 MHz) in the direction towards the Gal…