4C 02.29 , the SIMBAD biblio

4C 02.29 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.06.06CEST09:59:32

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1966AuJPh..19...35D 541 112 The Parkes catalogue of radio sources. Declination zone 0 to +20. DAY G.A., SHIMMINS A.J., EKERS R.D., et al.
1966AuJPh..19..649S 642 54 Accurate positions of 644 radio sources. SHIMMINS A.J., CLARKE M.E. and EKERS R.D.
1971AuJPA..19....1W 797 63 The Parkes 2700 MHz survey catalogues for the ±4 declination zone and for selected regions. WALL J.V., SHIMMINS A.J. and MERKELIJN J.K.
1974AJ.....79..437C 384 61 Intensity dependent radio spectral distributions in the Parkes 2700-MHz survey. CONDON J.J. and JAUNCEY D.L.
1975MmRAS..80....1M 340 68 Accurate positions and identifications for a complete sample of 341 radio sources from the Parkes ± 4 degres survey. McEWAN N.J., BROWNE I.W.A. and CROWTHER J.H.
1980A&AS...41...21G 357 6 Observations at 408 MHz of sources in the ±4 declination strip of the Parkes 2700-MHz survey. GRUEFF G., MACCACARO T. and WALL J.V.
1983ApJ...269..387P 102 15 A statistical VLBI study of milli-arcsecond cores in extragalactic radio sources. PRESTON R.A., MORABITO D.D. and JAUNCEY D.L.
1983ApJS...51...67L viz 237 24 5 GHz observations of sources in the Arecibo 611 MHz survey. LAWRENCE C.R., BENNETT C.L., GARCIA-BARRETO J.A., et al.
1985AJ.....90.1599P 1228 160 A VLBI survey at 2.29 GHz. PRESTON R.A., MORABITO D.D., WILLIAMS J.G., et al.
1986ApJS...61..105L 949 82 5 GHz radio structure and optical identifications of sources from the MG survey. II. Maps and finding charts. LAWRENCE C.R., BENNETT C.L., HEWITT J.N., et al.
1992A&A...264..203G 143 17 Low-frequency variability and the galactic distribution of electron-density fluctuation. GHOSH T. and RAO A.P.
1995AuJPh..48..143S viz 2214 69 Radio sources observed with the Culgoora circular array. SLEE O.B.
2003AJ....126.2125Z viz 291 306 Candidate type II quasars from the Sloan Digital Sky Survey. I. Selection and optical properties of a sample at 0.3<z<0.83. ZAKAMSKA N.L., STRAUSS M.A., KROLIK J.H., et al.
2004AJ....128.1002Z viz 177 92 Candidate type II quasars from the Sloan Digital Sky Survey. II. From radio to x-rays. ZAKAMSKA N.L., STRAUSS M.A., HECKMAN T.M., et al.
2006A&A...455..773V viz 108224 628 A catalogue of quasars and active nuclei: 12th edition. VERON-CETTY M.-P. and VERON P.
2008MNRAS.390..819G viz 15       D               279 15 The Combined NVSS-FIRST Galaxies (CoNFIG) sample - I. Sample definition, classification and evolution. GENDRE M.A. and WALL J.V.
2008AJ....136.2373R viz 890 251 Space density of optically selected type 2 quasars. REYES R., ZAKAMSKA N.L., STRAUSS M.A., et al.
2010A&A...511A..53V viz 15       D               1 107939 39 The SPECFIND V2.0 catalogue of radio cross-identifications and spectra. SPECFIND meets the Virtual Observatory. VOLLMER B., GASSMANN B., DERRIERE S., et al.
2010A&A...518A..10V viz 15       D               1 168912 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
2014ApJ...787...65H 212       D     X C       5 32 44 Gemini long-slit observations of luminous obscured quasars: further evidence for an upper limit on the size of the narrow-line region. HAINLINE K.N., HICKOX R.C., GREENE J.E., et al.
2014ApJS..212...15F viz 16       D               1 24940 60 A broadband polarization catalog of extragalactic radio sources. FARNES J.S., GAENSLER B.M. and CARRETTI E.
2018ApJ...859..116K viz 16       D               1 888 24 The black hole masses and Eddington ratios of type 2 quasars. KONG M. and HO L.C.
2019MNRAS.484.1021O viz 17       D               1 2523 ~ The redshift distribution of infrared-faint radio sources. ORENSTEIN B.J., COLLIER J.D. and NORRIS R.P.
2021A&A...655A..17S viz 17       D               1 338596 3 The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. STEIN Y., VOLLMER B., BOCH T., et al.

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