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Cosmic Flows: Green Bank Telescope and Parkes H i observations

Identifieur interne : 002C43 ( Istex/Curation ); précédent : 002C42; suivant : 002C44

Cosmic Flows: Green Bank Telescope and Parkes H i observations

Auteurs : Hélène M. Courtois [France, États-Unis] ; R. Brent Tully [États-Unis] ; D. I. Makarov [France, Russie] ; S. Mitronova [Russie] ; B. Koribalski [Australie] ; I. D. Karachentsev [France, Russie] ; J. Richard Fisher [États-Unis]

Source :

Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011-07-01.

RBID : ISTEX:EB928087E31BFADC566587C680C0569D5044527B

English descriptors

Abstract

The neutral hydrogen properties of 1822 galaxies are being studied with the Green Bank 100‐m and the Parkes 64‐m telescopes as part of the ‘Cosmic Flows’ programme. Observed parameters include systemic velocities, profile linewidths and integrated fluxes. The linewidth information can be combined with the optical and infrared photometry to obtain distances. The 1822 H i observations complement an inventory of archives. All told, H i linewidth information is available for almost all of five samples: (i) luminosity–linewidth correlation calibrators; (ii) zero‐point calibrators for the Type Ia supernova scale; (iii) a dense local sample of spiral galaxies with within 3000 km s−1; (iv) a sparser sample of 60‐μm selected galaxies within 6000 km s−1 that provides an all‐sky coverage of our extended supercluster complex; and (v) an even sparser sample of flat galaxies, extreme edge‐on spirals, extending in a volume out to 12 000 km s−1. The H i information for 13 941 galaxies, whether from the archives or acquired as part of the Cosmic Flows observational programme, is uniformly re‐measured and made available through the Extragalactic Distance Database website.

Url:

https://api.istex.fr/document/EB928087E31BFADC566587C680C0569D5044527B/fulltext/pdf

DOI: 10.1111/j.1365-2966.2011.18515.x

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<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Accurate linewidth measurements</term>
<term>Accurate measurements</term>
<term>Adhi</term>
<term>Adhi catalogue</term>
<term>Alfalfa</term>
<term>Alfalfa survey</term>
<term>Analog</term>
<term>Archival data</term>
<term>Archival material</term>
<term>Archive</term>
<term>Arecibo</term>
<term>Arecibo range</term>
<term>Arecibo telescope</term>
<term>Axial ratio</term>
<term>Black histogram</term>
<term>Blind surveys</term>
<term>Bottom panel</term>
<term>Cent completion</term>
<term>Cent level</term>
<term>Cosmic flows</term>
<term>Cosmic flows observations</term>
<term>Cosmic flows programme</term>
<term>Cosmic flows project</term>
<term>Courtois</term>
<term>Digital spectra</term>
<term>Distance measures</term>
<term>Faint limit</term>
<term>Flat galaxies</term>
<term>Flat galaxy catalog</term>
<term>Flat galaxy sample</term>
<term>Galactic latitudes</term>
<term>Galaxy</term>
<term>Galaxy distances</term>
<term>Galaxy luminosity</term>
<term>Galaxy motions</term>
<term>Galaxy properties</term>
<term>Giovanelli</term>
<term>Good coverage</term>
<term>Half power</term>
<term>Heliocentric recession velocity</term>
<term>Heliocentric velocity</term>
<term>High level</term>
<term>Histogram</term>
<term>Integration times</term>
<term>Large numbers</term>
<term>Large program</term>
<term>Large volume</term>
<term>Linewidth</term>
<term>Linewidth information</term>
<term>Linewidth measure</term>
<term>Linewidth parameters</term>
<term>Linewidths</term>
<term>Lower line</term>
<term>Lund astron</term>
<term>Malmquist</term>
<term>Mnras</term>
<term>Monthly notices</term>
<term>National radio astronomy observatory</term>
<term>Nearby galaxies</term>
<term>Neutral hydrogen properties</term>
<term>Normal spirals</term>
<term>Online version</term>
<term>Parkes</term>
<term>Parkes radiotelescope</term>
<term>Parkes telescope</term>
<term>Parkes telescopes</term>
<term>Peculiar velocities</term>
<term>Photometry</term>
<term>Programme</term>
<term>Pscz</term>
<term>Pscz sample</term>
<term>Radial velocity</term>
<term>Redshift</term>
<term>Rfgc</term>
<term>Rfgc galaxies</term>
<term>Rotation rate</term>
<term>Snia</term>
<term>Snia host galaxy sample</term>
<term>Solid line</term>
<term>Sparser sample</term>
<term>Spiral galaxies</term>
<term>Surface photometry</term>
<term>Telescope</term>
<term>Thick slice</term>
<term>Tidal disruption</term>
<term>Tully</term>
<term>Tully fisher</term>
<term>Valuable support</term>
<term>Various samples</term>
<term>Velocity measures</term>
<term>White histogram</term>
<term>Willick</term>
</keywords>
<keywords scheme="Teeft" xml:lang="en"><term>Accurate linewidth measurements</term>
<term>Accurate measurements</term>
<term>Adhi</term>
<term>Adhi catalogue</term>
<term>Alfalfa</term>
<term>Alfalfa survey</term>
<term>Analog</term>
<term>Archival data</term>
<term>Archival material</term>
<term>Archive</term>
<term>Arecibo</term>
<term>Arecibo range</term>
<term>Arecibo telescope</term>
<term>Axial ratio</term>
<term>Black histogram</term>
<term>Blind surveys</term>
<term>Bottom panel</term>
<term>Cent completion</term>
<term>Cent level</term>
<term>Cosmic flows</term>
<term>Cosmic flows observations</term>
<term>Cosmic flows programme</term>
<term>Cosmic flows project</term>
<term>Courtois</term>
<term>Digital spectra</term>
<term>Distance measures</term>
<term>Faint limit</term>
<term>Flat galaxies</term>
<term>Flat galaxy catalog</term>
<term>Flat galaxy sample</term>
<term>Galactic latitudes</term>
<term>Galaxy</term>
<term>Galaxy distances</term>
<term>Galaxy luminosity</term>
<term>Galaxy motions</term>
<term>Galaxy properties</term>
<term>Giovanelli</term>
<term>Good coverage</term>
<term>Half power</term>
<term>Heliocentric recession velocity</term>
<term>Heliocentric velocity</term>
<term>High level</term>
<term>Histogram</term>
<term>Integration times</term>
<term>Large numbers</term>
<term>Large program</term>
<term>Large volume</term>
<term>Linewidth</term>
<term>Linewidth information</term>
<term>Linewidth measure</term>
<term>Linewidth parameters</term>
<term>Linewidths</term>
<term>Lower line</term>
<term>Lund astron</term>
<term>Malmquist</term>
<term>Mnras</term>
<term>Monthly notices</term>
<term>National radio astronomy observatory</term>
<term>Nearby galaxies</term>
<term>Neutral hydrogen properties</term>
<term>Normal spirals</term>
<term>Online version</term>
<term>Parkes</term>
<term>Parkes radiotelescope</term>
<term>Parkes telescope</term>
<term>Parkes telescopes</term>
<term>Peculiar velocities</term>
<term>Photometry</term>
<term>Programme</term>
<term>Pscz</term>
<term>Pscz sample</term>
<term>Radial velocity</term>
<term>Redshift</term>
<term>Rfgc</term>
<term>Rfgc galaxies</term>
<term>Rotation rate</term>
<term>Snia</term>
<term>Snia host galaxy sample</term>
<term>Solid line</term>
<term>Sparser sample</term>
<term>Spiral galaxies</term>
<term>Surface photometry</term>
<term>Telescope</term>
<term>Thick slice</term>
<term>Tidal disruption</term>
<term>Tully</term>
<term>Tully fisher</term>
<term>Valuable support</term>
<term>Various samples</term>
<term>Velocity measures</term>
<term>White histogram</term>
<term>Willick</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">The neutral hydrogen properties of 1822 galaxies are being studied with the Green Bank 100‐m and the Parkes 64‐m telescopes as part of the ‘Cosmic Flows’ programme. Observed parameters include systemic velocities, profile linewidths and integrated fluxes. The linewidth information can be combined with the optical and infrared photometry to obtain distances. The 1822 H i observations complement an inventory of archives. All told, H i linewidth information is available for almost all of five samples: (i) luminosity–linewidth correlation calibrators; (ii) zero‐point calibrators for the Type Ia supernova scale; (iii) a dense local sample of spiral galaxies with within 3000 km s−1; (iv) a sparser sample of 60‐μm selected galaxies within 6000 km s−1 that provides an all‐sky coverage of our extended supercluster complex; and (v) an even sparser sample of flat galaxies, extreme edge‐on spirals, extending in a volume out to 12 000 km s−1. The H i information for 13 941 galaxies, whether from the archives or acquired as part of the Cosmic Flows observational programme, is uniformly re‐measured and made available through the Extragalactic Distance Database website.</div>
</front>
</TEI>
</record>

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Cosmic Flows: Green Bank Telescope and Parkes H i observations

Cosmic Flows: Green Bank Telescope and Parkes H i observations

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