4C 35.56 , the SIMBAD biblio

4C 35.56 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST02:06:06


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Title First 3 Authors
1967AJ.....72..738O 492 52 Accurate positions of selected 4C sources. OLSEN E.T.
1970AJ.....75..764O 487 125 Optical identification of radio sources selected from the 4C catalogue. OLSEN E.T.
1973ApJ...182L..13S 51 69 Redshifts for 51 galaxies identified with radio sources in the 4C catalog. SARGENT W.L.W.
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.
1979AJ.....84..437R 68 23 4C radio galaxies: structures and optical identifications. RUDNICK L. and ADAMS M.T.
1979AJ.....84.1111G 90 13 Extended radio sources and elliptical galaxies. III. Optical positions for galaxy centers. GOODSON R.E., PALIMAKA J.J. and BRIDLE A.H.
1980A&AS...40..191V 189 5 A study of the 4C catalogue of radio sources, between declinations 20 deg and 40 deg. II - The sample. VERON M.P. and VERON P.
1981MNRAS.196..669W 46 34 Optical and radio properties of 4C galaxies. WILKINSON A., HINE R.G. and SARGENT W.L.W.
1994A&AS..106..303N viz 242 37 Multifrequency observations of ROSAT selected radio sources. NEUMANN M., REICH W., FUERST E., et al.
1995A&AS..109..147B viz 629 94 The ROSAT AGN content of the 87GB 5 GHz survey: bulk properties of previously optically identified sources. BRINKMANN W., SIEBERT J., REICH W., et al.
2000A&A...363..141R viz 752 25 Radio-loud active galaxies in the northern ROSAT All-Sky Survey. IV. Properties of sources stronger than 100 mJy at 5 GHz. REICH W., FUERST E., REICH P., et al.
2010A&A...511A..53V viz 15       D               1 107473 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.
2023ApJS..268...31P 958     A D S   X C       21 33 ~ The Multiwavelength Environment of Second Bologna Catalog Sources. PAGGI A., MASSARO F., PENA-HERAZO H., et al.

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