Field IDField IDs are defined as: 0 = EN1, 1 = EN2, 2 = Lockman, 3 = SWIRE-VVDS, 4 = SWIRE-SXDS, 5 = XMM, 6 = CDFS, 7 = ELAIS-S1, 8 = Phoenix SIDNote that SID is NOT unique between the CDFS and ELAIS-S1 fields - use the "Field ID" to distinguish them. RA (HMS)HMS and DMS values for RA and Dec are now determined from the RA and Dec in degrees. For some yet to be determined reason, this produces coordinates which differ slightly in the last digit compared to the published values of the CDFS field. Dec (DMS)HMS and DMS values for RA and Dec are now determined from the RA and Dec in degrees. For some yet to be determined reason, this produces coordinates which differ slightly in the last digit compared to the published values of the CDFS field. RA (deg)CDFS: In the case of single-component sources, the source position is the radio position of the component. In the case of a complex source, such as a radio double, this is the position of the host galaxy. In the latter case this is the optical position if one is available, or else the SWIRE3 position. Dec (deg)CDFS: In the case of single-component sources, the source position is the radio position of the component. In the case of a complex source, such as a radio double, this is the position of the host galaxy. In the latter case this is the optical position if one is available, or else the SWIRE3 position. ClassCDFS: Class taken directly from published paper (Norris et al. 2006). ELAIS: Only AGN classification available. BasisCDFS: Basis taken directly from published paper (Norris et al. 2006). ELAIS: AGN classification from FIR-radio correlation when S24um(uJy) / (S20cm(Jy)*1e6) < 0.69. zSpecInternally, several spectroscopic redshift references are specified for some redshifts. Only the last listed reference is displayed for "zSpec Ref". zSpec RefInternally, several spectroscopic redshift references are specified for some redshifts. Only the last listed reference is displayed for "zSpec Ref".
SUMSS S36 cmSUMSS cross-identification is determined by performing a 5 arcsec radius cone-searches against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. VLA S20 cmVLA-ECDFS cross-identification is determined by performing a 1 arcsec radius cone-searches against the SWIRE3 position (where available) or the radio position.
S3IDCDFS: Data for SWIRE3 sources cross-identified against ATLAS sources are taken from the SWIRE3 catalogue, or where a numerical ID is specified, from a pre-release version of the SWIRE3 catalogue. The SWIRE3 cross-identification is taken from the published paper (Norris et al. 2006). F3.6 umFlux measurements are taken from flux_kr if ext_fl=2, otherwise they are taken from flux_ap2. F4.5 umFlux measurements are taken from flux_kr if ext_fl=2, otherwise they are taken from flux_ap2. F5.8 umFlux measurements are taken from flux_kr if ext_fl=2, otherwise they are taken from flux_ap2. F8.0 umFlux measurements are taken from flux_kr if ext_fl=2, otherwise they are taken from flux_ap2. F24 umFlux measurements are taken from flux_ap2. mbMagnitudes are taken from kr_m_b if stell_b<0.2, otherwise they are taken from ap_m_b. mvMagnitudes are taken from kr_m_v if stell_v<0.2, otherwise they are taken from ap_m_v. mrMagnitudes are taken from kr_m_r if stell_r<0.2, otherwise they are taken from ap_m_r.
S4IDData for SWIRE4 sources cross-identified against ELAIS-S1 sources are taken from a pre-release version of the SWIRE4 catalogue. The SWIRE4 cross-identifications are taken directly from the published paper (Middelberg et al. 2008). F3.6 umFlux measurements are taken from flux_kr if ext_fl=2, otherwise they are taken from flux_ap2. F4.5 umFlux measurements are taken from flux_kr if ext_fl=2, otherwise they are taken from flux_ap2. F5.8 umFlux measurements are taken from flux_kr if ext_fl=2, otherwise they are taken from flux_ap2. F8.0 umFlux measurements are taken from flux_kr if ext_fl=2, otherwise they are taken from flux_ap2. F24 umFlux measurements are taken from flux_ap2. mbMagnitudes are taken from kr_m_b if stell_b<0.2, otherwise they are taken from ap_m_b. mvMagnitudes are taken from kr_m_v if stell_v<0.2, otherwise they are taken from ap_m_v. mrMagnitudes are taken from kr_m_r if stell_r<0.2, otherwise they are taken from ap_m_r.
70 um IDSWIRE2 cross-identification is determined by performing a 5 arcsec radius cone-searches against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. 160 um IDSWIRE2 cross-identification is determined by performing a 9 arcsec radius cone-searches against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position.
I IDESIS cross-identifications are determined by performing 2 arcsec radius cone-search against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. mIESIS I magnitude is taken from the Imag field of the catalogue. z IDESIS cross-identifications are determined by performing 2 arcsec radius cone-search against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. mzESIS z magnitude is taken from the zmag field of the catalogue.
RRIDRowan-Robinson cross-identifications are determined by performing 1 arcsec radius cone-searches against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. zPhotThe redshift is calculated from alz if err0 < err1, otherwise it is calculated from alz2.
SCIDSuperCOSMOS cross-identifications are determined by performing 1 arcsec radius cone-searches against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position.
1Ms XIDChandra cross-identifications are determined by performing 4 arcsec radius cone-searches against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. 2Ms XIDChandra cross-identifications are determined by performing 1 arcsec radius cone-searches against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position.
MUSYC-ECDFS zSpecMUSYC-ECDFS cross-identifications are determined by performing 1 arcsec radius conesearch against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. AAOSLzAAOSLz cross-identifications are determined by performing 1 arcsec radius conesearch against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. AAOzAAOz cross-identifications are determined by performing 1 arcsec radius conesearch against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. COMBO17 MCzCOMBO17 cross-identifications are determined by performing 1 arcsec radius conesearch against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. FIREWORKS zph_bestFIREWORKS cross-identifications are determined by performing 1 arcsec radius conesearch against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. GOODSzGOODSz cross-identifications are determined by performing 1 arcsec radius conesearch against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position. GOODSVIMOSzGOODSVIMOSz cross-identifications are determined by performing 1 arcsec radius conesearch against the SWIRE4 position (where available), SWIRE3 position (where available) and finally the radio position.