Optical identification of radio sources with the I band CCD catalogue





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positions limit of the I band catalogue used for the cross correlation:
35.8051 < RA < 37.1931 -4.97655 < DEC < -4.02486
02 23 13.22 < RA < 02 28 46.34 -04 58 35.58 < DEC < -04 01 29.5

Area covered : about 1.31 deg2
(extremely approsimated value obtained from the RA and DEC limit of the I band catalogue)

Optical sources in the catalogue : 170488 (~130000 sources/deg2)
Radio sources within I band CCD area : 1060

Histogram of the number of optical sources
within a radius of 10 arcsec around each radio position




  1. As first step we used 2 arcsec for the radio-optical associations.
    Using r=2arcsec we have 832 associations

    Using these 832 associations we have :
    Mean offsets (arcsec)
    RADIO - I Band position RA, DEC: 0.09 , 0.30
    Median offsets (arcsec)
    RADIO - I Band position RA, DEC: 0.12 , 0.32
    Standard deviation RA, DEC: 0.56 , 0.63

    Position offset between radio and optical position


  2. As second step we applied the median offset values to the radio positions (i.e. we corrected the radio position of RA : -0.12 arcsec and DEC : -0.32) and we cross-correlated again the radio and optical catalogues.
    Here there is the histogram of the number of optical sources
    again within a radius of 10 arcsec around each radio position (offset corrected)

  3. Finally we used a radius of 1.5 arcsec around each radio position to find the optical counterparts. Using r=1.5 arcsec we have 755 associations, 78 of which (9.9 per cent) are expected to be spurious associations
    Click here for the list of the 755 associations


    So.. as preliminary results we have : 755 - 78 = 677 likely associations ( ==> 677 / 1060 = 64 % of the radio sources within CCD area)

    Position offset between radio (offset corrected) and optical position



    I band magnitude distribution of the whole catalogue and of the 755 optical counterparts of the radio sources


    I band magnitude distribution of the 755 optical counterparts of the radio sources and the expected magnitude distribution of the spurious sources


    Radio flux distribution of the whole radio catalogue and of the radio sources with an optical id


Published by Paolo Ciliegi, paolo@avalon.bo.astro.it
Last modified: Fri Jun 22 13:03:18 CEST 2001