4C 37.44 , the SIMBAD biblio

4C 37.44 , the SIMBAD biblio (25 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST03:03:26

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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
1966MNRAS.134..371L 262 52 The radio spectra of sources in the fourth Cambridge catalogue. LONG R.J., SMITH M.A., STEWART P., et al.
1967AJ.....72..536S 274 55 A High-Sensivity Survey of the North Polar Galactic Region at 1415 MHz. SCHEER D.J. and KRAUS J.D.
1967AJ.....72..738O 492 52 Accurate positions of selected 4C sources. OLSEN E.T.
1967MNRAS.135..361S 195 13 Further radio studies of sources in the fourth Cambridge catalogue. STEWART P. and LONG R.J.
1969AJ.....74..833H 199 10 Declination measurements of selected 4C sources using the Arecibo 1000-ft reflector. HAZARD C., JAUNCEY D.L., GULKIS S., et al.
1970AJ.....75..764O 487 125 Optical identification of radio sources selected from the 4C catalogue. OLSEN E.T.
1970AJ.....75.1039H 73 35 The identification of 4C sources usung the 4C right ascensions and Arecibo declinations. HAZARD C., JAUNCEY D.L. and BACKER D.C.
1972A&A....16..379B 162 5 Results of an initial survey structure in radio sources at 81.5 MHz. BURNELL S.J.
1975AJ.....80..335S 1095 38 Positions and flux densities of 1075 radio sources at 365 MHz. SHARP J.R. and BASH F.N.
1977A&AS...27..155C 73 39 Measurements of structure and polarization of 72 sources from the 4C catalogue. CONWAY R.G., BURN B.J. and VALLEE J.P.
1977A&AS...27..171P 72 21 Optical identification of a sample of 4C sources. PADRIELLI L. and CONWAY R.G.
1978AJ.....83..451P 489 164 The 5-GHz strong source surveys. IV. Survey of the area between declination 35 and 70deg and summary of source counts, spectra and optical identifications. PAULINY-TOTH I.I.K., WITZEL A., PREUSS E., et al.
1978AcA....28..367M viz 2024 27 The Green Bank second survey of extragalactic radio sources at 1400 MHz. The catalogue of sources. MACHALSKI J.
1979A&AS...35..371G 197 21 Optical identification and 5GHz flux measurements of radiosources selected from the B2 catalogue -V. GRUEFF G. and VIGOTTI M.
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.
1980A&AS...40...91K 189 73 Statistical properties of radio sources of intermediate strength. KATGERT-MERKELIJN J., LARI C. and PADRIELLI L.
1982AJ.....87.1132M 248 23 A complete sample of intermediate-strength radio sources selected from the GB/GB2 1400-MHz surveys. I. Radio spectra and optical identifications of sources stronger than 0.55 Jy. MACHALSKI J. and MASLOWSKI J.
1990A&AS...82...41K viz 751 14 Spectral index distribution for a sample of sources from the B3 catalogue. KULKARNI V.K., MANTOVANI F. and PAULINY-TOTH I.I.K.
1998A&AS..128..153M viz 405 15 The revised GB/GB2 sample of extragalactic radio sources. MACHALSKI J.
2003KFNT...19d.291B 187 ~ Decametric survey of discrete sources in the northern sky. XIIIb. Spectra of discrete sources in the declination zone from +30 deg. to 40 deg. BRAUDE S.Y., MIROSHNICHENKO A.P., RASHKOVSKII S.L., et al.
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.
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.
2016A&A...586A.117P 16       D               1 112 13 A study of a sample of high rotation-measure AGNs through multifrequency single-dish observations. PASETTO A., KRAUS A., MACK K.-H., et al.
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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