/ftp/cats/aliases/P/1PSZ



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VIII/91       Planck Catalog of Compact Sources Release 1     (Planck, 2013)
The following files can be converted to FITS (extension .fit or fit.gz)
	f*.dat psz1.dat notes.dat
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Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=VIII/91
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drwxr-xr-x 103 cats archive 4096 May 11 11:42 [Up] drwxr-xr-x 8 cats archive 4096 Dec 22 2015 [TAR file] -rw-r--r-- 1 cats archive 471 Dec 22 2015 .message -r--r--r-- 1 cats archive 13562 May 12 2015 ReadMe -rw-r--r-- 1 cats archive 3186 Dec 22 2015 +footg5.gif -rw-r--r-- 1 cats archive 51097 Dec 22 2015 +footg8.gif drwxr-xr-x 2 cats archive 98 Apr 12 2013 doc -r--r--r-- 1 cats archive 83688 Apr 11 2013 f030.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 44609 Apr 11 2013 f044.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 58373 Apr 11 2013 f070.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 230177 Apr 11 2013 f100.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 339008 Apr 11 2013 f143.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 940054 Apr 11 2013 f217.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 862978 Apr 11 2013 f353.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1063277 Apr 11 2013 f545.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1956532 Apr 11 2013 f857.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] drwxr-xr-x 2 cats archive 4096 Apr 12 2013 fits -r--r--r-- 1 cats archive 6744 Apr 11 2013 notes.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 48200 Apr 11 2013 psz1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] drwxr-xr-x 12 cats archive 4096 Feb 16 2011 stamps
Beginning of ReadMe : VIII/91 Planck Catalog of Compact Sources Release 1 (Planck, 2013) ================================================================================ Planck Compact Source Catalogue Public Release 1 Planck Collaboration <Astron. Astrophys. 571, A29> =2014A&A...571A..29P =2013yCat.8091....0P ================================================================================ ADC_Keywords: Millimetric/submm sources ; Surveys Mission_Name: Planck Keywords: cosmology: observations ; surveys ; catalogues ; radio continuum: general ; submillimeter: general Description: Planck is a European Space Agency (ESA) mission, with significant contributions from the U.S. National Aeronautics and Space Agency (NASA). It is the third generation of space-based cosmic microwave background experiments, after the Cosmic Background Explorer (COBE) and the Wilkinson Microwave Anisotropy Probe (WMAP). Planck was launched on 14 May 2009 on an Ariane 5 rocket from Kourou, French Guiana. Following a cruise to the Earth-Sun L2 Lagrange point, cooling and in orbit checkout, Planck initiated the First Light Survey on 13 August 2009. Since then, Planck has been continuously measuring the intensity of the sky over a range of frequencies from 30 to 857GHz (wavelengths of 1cm to 350mum) with spatial resolutions ranging from about 33' to 5' respectively. The Low Frequency Instrument (LFI) on Planck provides temperature and polarization information using radiometers which operate between 30 and 70GHz. The High Frequency Instrument (HFI) uses pairs of polarization-sensitive bolometers at each of four frequencies between 100 and 353GHz but does not measure polarization information in the two upper HFI bands at 545 and 857GHz. The lowest frequencies overlap with WMAP, and the highest frequencies extend far into the submillimeter in order to improve separation between Galactic foregrounds and the cosmic microwave background (CMB). By extending to wavelengths longer than those at which the Infrared Astronomical Satellite (IRAS) operated, Planck is providing an unprecedented window into dust emission at far-infrared and submillimeter wavelengths. The PCCS (Planck Catalog of Compact Sources) is the list of sources detected in the first 15 months of Planck "nominal" mission. It consists of nine single-frequency catalogues of compact sources, both Galactic and extragalactic, detected over the entire sky. The PCCS covers the frequency range 30-857 GHz with higher sensitivity (it is 90% complete at 180mJy in the best channel) and better angular resolution than previous all-sky surveys in the microwave band. By construction its reliability is >80% and more than 65% of the sources have been detected at least in two contiguous Planck channels. Many of the Planck PCCS sources can be associated with stars with dust shells, stellar cores, radio galaxies, blazars, infrared luminous galaxies and Galactic interstellar medium features.

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