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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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Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2017★ 23 cited

A deep Parkes HI survey of the Sculptor group and filament: HI mass function and environment

T. Westmeier, D. Obreschkow, M. Calabretta +8

We present the results of a deep survey of the nearby Sculptor group and the associated Sculptor filament taken with the Parkes 64-m radio telescope in the 21-cm emission line of n…

astro-ph.GA2016★ 1.6k cited

HI4PI: A full-sky HI survey based on EBHIS and GASS

HI4PI Collaboration, N. Ben Bekhti, L. Flöer +18

Measurement of the Galactic neutral atomic hydrogen (HI) column density, NHI, and brightness temperatures, Tb, is of high scientific value for a broad range of astrophysical discip…

astro-ph.GA2015★ 30 cited

On the neutral gas content of nine new Milky Way satellite galaxy candidates

T. Westmeier, L. Staveley-Smith, M. Calabretta +5

We use a new, improved version of the HI Parkes All-Sky Survey to search for HI emission from nine new, ultra-faint Milky Way satellite galaxy candidates recently discovered in dat…

astro-ph.GA2015★ 1 cited

A blind HI Mass Function from the Arecibo Ultra-Deep Survey (AUDS)

L. Hoppmann, L. Staveley-Smith, W. Freudling +3

The Arecibo Ultra Deep Survey (AUDS) combines the unique sensitivity of the telescope with the wide field of the Arecibo L-band Feed Array (ALFA) to directly detect 21cm HI emissio…

astro-ph.GA2014★ 90 cited

The HIPASS survey of the Galactic plane in Radio Recombination Lines

Marta I. R. Alves, Mark Calabretta, Rodney D. Davies +5

We present a Radio Recombination Line (RRL) survey of the Galactic Plane from the HI Parkes All-sky Survey and associated Zone of Avoidance survey, which mapped the region l=196deg…

astro-ph.GA2011★ 58 cited

A derivation of the free-free emission on the Galactic plane between l=20 and 44 degrees

Marta I. R. Alves, Rodney D. Davies, Clive Dickinson +3

We present the derivation of the free-free emission on the Galactic plane between l=20 and 44 degrees and |b| < 4 degrees, using Radio Recombination Line (RRL) data from the HI Par…