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20022017
most citedHI4PI: A full-sky HI survey based on EBHIS and GASS

1.6k citations · 4.7k across the 25 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008★ 35 cited

HI Clouds in the Lower Halo: I. The Galactic All-Sky Survey Pilot Region

H. Alyson Ford, N. M. McClure-Griffiths, Felix J. Lockman +5

We have detected over 400 HI clouds in the lower halo of the Galaxy within the pilot region of the Galactic All-Sky Survey (GASS), a region of the fourth quadrant that spans 18 deg…

astro-ph2007★ 53 cited

An Interaction of a Magellanic Leading Arm High Velocity Cloud with the Milky Way Disk

N. M. McClure-Griffiths, L. Staveley-Smith, F. J. Lockman +6

The Leading Arm of the Magellanic System is a tidally formed HI feature extending $\sim 60\arcdeg$ from the Magellanic Clouds ahead of their direction of motion. Using atomic hydro…

astro-ph2005★ 54 cited

Evidence for chimney breakout in the Galactic supershell GSH 242-03+37

N. M. McClure-Griffiths, A. Ford, D. J. Pisano +5

We present new high resolution neutral hydrogen (H I) images of the Galactic supershell GSH 242-03+37. These data were obtained with the Parkes Radiotelescope as part of the Galact…

astro-ph2005★ 87 cited

Representations of spectral coordinates in FITS

E. W. Greisen, M. R. Calabretta, F. G. Valdes +1

Greisen & Calabretta describe a generalized method for specifying the coordinates of FITS data samples. Following that general method, Calabretta & Greisen describe detailed conven…

astro-ph2004★ 527 cited

The 1000 Brightest HIPASS Galaxies: HI Properties

B. S. Koribalski, L. Staveley-Smith, V. A. Kilborn +5

(abridged) We present the HIPASS Bright Galaxy Catalog (BGC) which contains the 1000 HI-brightest galaxies in the southern sky as obtained from the HI Parkes All-Sky Survey (HIPASS…

astro-ph2002★ 253 cited

A New Look at the Large-Scale HI Structure of the LMC

L. Staveley-Smith, S. Kim, M. R. Calabretta +2

We present a Parkes multibeam \HI survey of the Large Magellanic Cloud (LMC). This survey, which is sensitive to spatial structure in the range 200 pc to 10 kpc, complements the Au…