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J/PASP/122/261 Herschel Reference Survey Sample (Boselli+, 2010)
The following files can be converted to FITS (extension .fit or fit.gz)
table1.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/PASP/122/261
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-r--r--r-- 1 cats archive 6263 Feb 1 2011 ReadMe
-rw-r--r-- 1 cats archive 446 Feb 1 2011 +footg5.gif
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-r--r--r-- 1 cats archive 40105 Apr 4 2010 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/PASP/122/261 Herschel Reference Survey Sample (Boselli+, 2010)
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The Herschel Reference Survey.
Boselli A., Eales S., Cortese L., Bendo G., Chanial P., Buat V., Davies J.,
Auld R., Rigby E., Baes M., Barlow M., Bock J., Bradford M.,
Castro-Rodriguez N., Charlot S., Clements D., Cormier D., Dwek E.,
Elbaz D., Galametz M., Galliano F., Gear W., Glenn J., Gomez H.,
Griffin M., Hony S., Isaak K., Levenson L., Lu N., Madden S.,
O'Halloran B., Okamura K., Oliver S., Page M., Panuzzo P., Papageorgiou A.,
Parkin T., Perez-Fournon I., Pohlen M., Rangwala N., Roussel H., Rykala A.,
Sacchi N., Sauvage M., Schulz B., Schirm M., Smith M.W.L., Spinoglio L.,
Stevens J., Symeonidis M., Vaccari M., Vigroux L., Wilson C., Wozniak H.,
Wright G., Zeilinger W.
<Publ. Astron. Soc. Pac. 122, 261 (2010)>
=2010PASP..122..261B
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ADC_Keywords: Galaxy catalogs ; Radial velocities ; Photometry, infrared
Abstract:
The Herschel Reference Survey is a Herschel guaranteed time key
project and will be a benchmark study of dust in the nearby universe.
The survey will complement a number of other Herschel key projects
including large cosmological surveys that trace dust in the distant
universe. We will use Herschel to produce images of a
statistically-complete sample of 323 galaxies at 250, 350, and 500um.
The sample is volume-limited, containing sources with distances
between 15 and 25Mpc and flux limits in the K band to minimize the
selection effects associated with dust and with young high-mass stars
and to introduce a selection in stellar mass. The sample spans the
whole range of morphological types (ellipticals to late-type spirals)
and environments (from the field to the center of the Virgo Cluster)
and as such will be useful for other purposes than our own. We plan to
use the survey to investigate (i) the dust content of galaxies as a
function of Hubble type, stellar mass, and environment; (ii) the
connection between the dust content and composition and the other
phases of the interstellar medium; and (iii) the origin and evolution
of dust in galaxies. In this article, we describe the goals of the
survey, the details of the sample and some of the auxiliary observing
programs that we have started to collect complementary data. We also
use the available multifrequency data to carry out an analysis of the
statistical properties of the sample.