4C 32.28 , the SIMBAD biblio

4C 32.28 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST06:34:31


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Title First 3 Authors
1967AJ.....72..738O 492 52 Accurate positions of selected 4C sources. OLSEN E.T.
1969A&A.....2..477F 136 17 The radiospectra of a homogeneous sample 4C radio sources. FANTI C., FANTI R., LONDRILLO P., et al.
1970AJ.....75..764O 487 125 Optical identification of radio sources selected from the 4C catalogue. OLSEN E.T.
1971AJ.....76..530G 226 15 Flux density measurements of optically identified B2 radio sources at 5 GHz. GRUEFF G.
1972A&AS....6....1G 356 76 Optical identification of radio-sources selected from the B2 catalogue. GRUEFF G. and VIGOTTI M.
1973AJ.....78....1D 628 61 First results from the Texas interferometer: positions of 605 discrete sources. DOUGLAS J.N., BASH F.N., GHIGO F.D., et al.
1979A&AS...36..331V 425 8 A study of the 4C catalogue of radio sources between declinations 20 and 40 degres. I. 318 MHz flux density measurements. VERON M.P. and VERON P.
2004MNRAS.354..485B viz 15       D               1 176 33 The radio source population at high frequency: follow-up of the 15-GHz 9C survey. BOLTON R.C., COTTER G., POOLEY G.G., et al.
2006A&A...449..985M         O           24 14 FIRST-based survey of compact steep spectrum sources. III. MERLIN and VLBI observations of subarcsecond-scale objects. MARECKI A., KUNERT-BAJRASZEWSKA M. and SPENCER R.E.
2010A&A...511A..53V viz 15       D               1 107940 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.
2010MNRAS.408.2261K viz 15       D               1 168 106 A survey of low-luminosity compact sources and its implication for the evolution of radio-loud active galactic nuclei - I. Radio data. KUNERT-BAJRASZEWSKA M., GAWRONSKI M.P., LABIANO A., et al.
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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