The HI Parkes All Sky Survey: southern observations, calibration and robust imaging

By David G. Barnes, L. Staveley-Smith, W. D. de Blok, T. Oosterloo, I. Stewart, A. Wright, G. Banks, R. Bhathal, P. Boyce, M. Calabretta and 29 more. 2001

492 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Computational Mechanics

View Paper: https://www.semanticscholar.org/paper/4e4eb21fb940a9d2001c60e3f8264dc6f216b345

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Citations in the corpus

GASS: THE PARKES GALACTIC ALL-SKY SURVEY. I. SURVEY DESCRIPTION, GOALS, AND INITIAL DATA RELEASE (2009, methodology): “The HIPASS survey (Barnes et al. 2001, Putman et al. 2002) covered the sky at ∼ 15′ resolution, but was not designed for Galactic H i, and therefore did not accurately measure low velocity gas, nor have the velocity resolution needed to resolve interstellar H i lines.”
Farthest Neighbor: The Distant Milky Way Satellite Eridanus II (2016, methodology): “However, Westmeier et al. (2015) measured the H I gas content using HIPASS data (Barnes et al. 2001), and did not detect any H I gas associated with Eri II.”
A Digital Archive of H I 21 Centimeter Line Spectra of Optically Targeted Galaxies (2005, background): “…notably the Arecibo HI Strip Survey (AHISS; Zwaan et al. 1997), the Arecibo Dual Beam Survey (ADBS; Rosenberg & Schneider 2000), the HI Jodrell All-Sky Survey (HIJASS; Lang et al. 2003) and the HI Parkes All-Sky Survey (HIPASS; Barnes et al. 2001; Koribalski et al. 2004; Meyer et al. 2004).”
THE GALFA-Hi SURVEY: DATA RELEASE 1 (2011, methodology): “PRO uses the core logic described in Dickey (2002) and many of the methods developed for Parkes gridzilla (Barnes et al. 2001) and the AIPS procedure SDGRID.”
THE ARECIBO LEGACY FAST ALFA SURVEY: THE α.40 H i SOURCE CATALOG, ITS CHARACTERISTICS AND THEIR IMPACT ON THE DERIVATION OF THE H i MASS FUNCTION (2011, background): “…of multi-feed array receivers on large single dish telescopes made possible wide-area 21 cm HI line surveys, such as the HI Parkes All-Sky Survey, (HIPASS: Barnes et al. 2001; Meyer et al. 2004; Wong et al. 2006) and – 3 – the companion HI Jodrell Bank All-Sky Survey (HIJASS: Lang et al. 2003).”
THE ARECIBO LEGACY FAST ALFA SURVEY: THE GALAXY POPULATION DETECTED BY ALFALFA (2012, methodology): “Compared to the HI Parkes All Sky Survey (HIPASS: Barnes et al. 2001; Meyer et al. 2004; Wong et al. 2006), ALFALFA is 8 times more sensitive, its spectral coverage extends over 1.6 times the bandwidth of HIPASS, and the angular resolution of ALFA is 4 times better than that of the Parkes multifeed…”
HI4PI: a full-sky H i survey based on EBHIS and GASS (2016, methodology): “Pre-processing of GASS data was performed using the Livedata package (Barnes et al. 2001), but for radio-frequency interference (RFI) mitigation, flux calibration, baseline fitting, and SR correction, dedicated software was used.”
The Magellanic Stream, High-Velocity Clouds, and the Sculptor Group (2002, methodology): “Again, see Barnes et al. 2001 for a full description of the gridding algorithm and the flux density correction for objects less than 30′ in size.”
Distances to nearby galaxies in Sculptor (2003, background): “The galaxy was not detected in the H i line by Côté et al. (1997), neither was it detected in the “blind” HIPASS survey by Staveley-Smith et al. (1998) and Barnes et al. (2001).”
xGASS: total cold gas scaling relations and molecular-to-atomic gas ratios of galaxies in the local Universe (2018, methodology): “Blind surveys of atomic hydrogen such as the H I Parkes All-Sky Survey (Barnes et al. 2001; Meyer et al. 2004; Wong et al. 2006), and the Arecibo Legacy Fast ALFA survey (ALFALFA; Giovanelli et al. 2005; Haynes et al. 2011) measured the H I content for ∼50 000 galaxies, but detect only the most gas-”
The Arecibo Legacy Fast ALFA Survey. I. Science Goals, Survey Design, and Strategy (2005, methodology): “It uses a HIPASS limit of 13.3 mJy per map pixel area, as reported by Barnes et al. (2001).”
The ATLAS3D project - XIII. Mass and morphology of H I in early-type galaxies as a function of environment (2011, methodology): “Recent progress in this kind of analysis has been made possible by single-dish blind surveys of large areas of the sky such as HIPASS (Barnes et al. 2001; see Sadler, Oosterloo & Morganti 2002 for an H I study of ETGs based on these data) and ALFALFA (Giovanelli et al. 2005).”
A new look at the large-scale H I structure of the Large Magellanic Cloud (2002, methodology): “Therefore, the beam was slightly broadened in the scan direction to 14.5 arcmin (Barnes et al. 2001).”
The Parkes HI survey of the Magellanic System (2004, methodology): “The second survey is the H Parkes All Sky Survey (HIPASS, Barnes et al. 2001), that was performed using the multi-beam facility of the Parkes telescope (Staveley-Smith et al. 1996).”
The 6-GHz multibeam maser survey-I. Techniques (2008, methodology): “The capabilities of this package, and its first use (in the HI Parkes All Sky Survey, HIPASS), have been described extensively by Barnes et al. (2001).”
HIPASS High-Velocity Clouds: Properties of the Compact and Extended Populations (2001, methodology): “+2◦ and within the lsr (Local Standard of Rest) velocity range −500 km s−1 to +500 km s−1, using data from the HI Parkes All-Sky Survey (Barnes et al. 2001), reduced with an algorithm which recovers extended emission (Putman et al. 2002; Putman 2000).”
The Origin of the Magellanic Stream and Its Leading Arm (2007, methodology): “For example, Putman et al. (1998) used the HIPASS data (Barnes et al. 2001) to discover a gaseous leading arm of the MS.”
An Hα Imaging Survey of Galaxies in the Local 11 Mpc Volume (2004, unknown): “…Galaxies (SINGG;Meurer et al. 2006), which is based on anH iY selected subsample of 468 z 0:0423 galaxies from theH i Parkes All Sky Survey (HIPASS; Barnes et al. 2001), the Analysis of the Interstellar Medium of Isolated Galaxies (AMIGA; VerdesMontenegro et al. 2005), which is observing a sample…”