ivo://astron.nl/lolss/q/source_catalogASTRONde Gasperin, F.Williams, W. L.Best, P.Bruggen, M.Brunetti, G.Cuciti, V.Dijkema, T. J.Hardcastle, M. J.Norden, M. J.Offringa , A.Shimwell, T.van Weeren, R.Bomans, D.Bonafede, A.Botteon, A.Callingham, J. R.Cassano, R.Chyzy, K. T.Emig, K. L.Edler, H.Haverkorn, M.Heald, G.Heesen, V.Iacobelli, M.Intema, H. T.Kadler, M.Malek, K.Mevius, M.Miley, G.Mingo, B.Morabito, L. K.Sabater, J.Morganti, R.Orru, E.Pizzo, R.Prandoni, I.Shulevski, A.Tasse, C.Vaccari, M.Zarka, P.Rottgering, H.2023-09-28T14:14:13Michael Sipior

Oude Hoogeveensedijk 4, 7991PD Dwingeloo, the Netherlands

vo@astron.nlradio-continuum-emissiondiscrete-radio-sources This page provides public access to the LBA survey of HETDEX, as a single mosaic over the HETDEX field and associated catalogue, covering around 700 square degrees centered in the RA range 10h45m00s to 15h30m00s and DEC range 45d00m00s to 57d00m00s. 25,247 sources are detected and the rms noise level is around 4 mJy/beam at a resolution of 47 arcsec and an effective frequency of 54 MHz. The flux scale appears to be good based on a comparison with VLSS.2021A&A...648A.104Dhttps://vo.astron.nl/tableinfo/lolss.source_catalogSurveyResearchLOFARLOFAR.LBA5/27772.78295e-26 4.37321e-23Radiololss This page provides public access to the LBA survey of HETDEX, as a single mosaic over the HETDEX field and associated catalogue, covering around 700 square degrees centered in the RA range 10h45m00s to 15h30m00s and DEC range 45d00m00s to 57d00m00s. 25,247 sources are detected and the rms noise level is around 4 mJy/beam at a resolution of 47 arcsec and an effective frequency of 54 MHz. The flux scale appears to be good based on a comparison with VLSS.lolss.source_catalog This page provides public access to the LBA survey of HETDEX, as a single mosaic over the HETDEX field and associated catalogue, covering around 700 square degrees centered in the RA range 10h45m00s to 15h30m00s and DEC range 45d00m00s to 57d00m00s. 25,247 sources are detected and the rms noise level is around 4 mJy/beam at a resolution of 47 arcsec and an effective frequency of 54 MHz. The flux scale appears to be good based on a comparison with VLSS.sourcemeta.id;meta.maincharnullableradegpos.eq.ra;meta.mainfloatindexednullabledecdegpos.eq.dec;meta.mainfloatindexednullablee_raarcsecpos.eq.ra;stat.errorfloatnullablee_decarcsecpos.eq.dec;stat.errorfloatnullabletot_fluxIntegrated flux densitymJyfloatnullablee_tot_fluxError on the integrated flux densitymJyfloatnullablepeak_fluxPeak brightness (affected by smearing)mJy/beamfloatnullablee_peak_fluxError on peak brightnessmJy/beamfloatnullablemaj_axisSource size, major axisarcsecfloatnullablee_majError on the major axis sizearcsecfloatnullablemin_axisSource size, minor axisarcsecfloatnullablee_minError on the minor axis sizearcsecfloatnullablepadegfloatnullablee_padegfloatnullabledc_majDeconvolved source size, major axisarcsecfloatnullablee_dc_majError on the deconvolved major axis sizearcsecfloatnullabledc_minDeconvolved source size, minor axisarcsecfloatnullablee_dc_minError on the deconvolved minor axis sizearcsecfloatnullabledc_padegfloatnullablee_dc_padegfloatnullableisl_rmsmJy/beamfloatnullables_code`S' indicates an isolated source which is fit with a single Gaussian; `C' represents sources that are fit by a single Gaussian but are within an island of emission that also contains other sources; and `M' is used for sources which are extended and fitted with multiple Gaussiansmeta.codecharnullable