/ftp/cats/aliases/P/PDS_3_



==========================================================================
J/MNRAS/296/839    Phoenix Deep Survey: 1.4-GHz source counts  (Hopkins+, 1998)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	pdf.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/cgi-bin/VizieR?-source=J/MNRAS/296/839
==========================================================================

drwxr-xr-x 4 cats archive 96 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 283 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 469 Dec 19 2022 .message -r--r--r-- 1 cats archive 6676 Oct 10 2000 ReadMe -rw-r--r-- 1 cats archive 1018 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2574 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 34068 Oct 2 2000 pdf.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/MNRAS/296/839 Phoenix Deep Survey: 1.4-GHz source counts (Hopkins+, 1998) ================================================================================ The Phoenix Deep Survey: 1.4-GHz source counts Hopkins A.M., Mobasher, B. Cram, L., Rowan-Robinson, M. <Mon. Not. R. Astron. Soc. 296, 839 (1998)> =1998MNRAS.296..839H ================================================================================ ADC_Keywords: Surveys ; Radio sources Keywords: surveys - galaxies: evolution - galaxies: luminosity function, mass function - radio continuum: galaxies Abstract: We present the first results from the Phoenix Deep Survey, a multiwavelength survey of a 2 deg diameter region. Observations in the radio continuum at 1.4 GHz carried out with the Australia Telescope Compact Array are described. The catalogue of over 1000 radio sources compiled from these observations is analyzed, and the source counts are presented. We model the observational source counts using a two-population model and published luminosity functions for these populations. Upon invoking luminosity and density evolution, we find that a luminosity evolution model best fits the radio observations, consistent with earlier work. The redshift distribution of the two galaxy populations investigated is also modeled and discussed.