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4C 16.68 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST06:54:23 |
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. | |||||
1967AJ.....72..757D | 628 | 52 | A survey of the sky at 610.5 MHz. II. The region between declinations +15 and +22 degrees. | DICKEL J.R., YANG K.S., McVITTIE G.C., et al. | |||||
1968AJ.....73..135G | 627 | 132 | Survey of radio sources observed in the continuum near 1420 MHz, declinations -5 to +70. | GALT J.A. and KENNEDY J.E.D. | |||||
1968MNRAS.139..289W | 373 | 34 | The radio spectra of sources in the fourth Cambridge catalogue -III. | WILLIAMS P.J.S., COLLINS R.A., CASWELL J.L., et al. | |||||
1972AJ.....77..405B | 574 | 259 | Flux densities, positions, and structures for a complete sample of intense radio sources at 1400 MHz. | BRIDLE A.H., DAVIS M.M. and FOMALONT E.B. | |||||
1977AJ.....82...21B | 456 | 21 | Variability of extragalactic sources at 2.7 GHz II. Flux densities of 550 sources and further evidence for variations. | BRIDLE A.H., KESTEVEN M.J.L. and BRANDIE G.W. | |||||
1995AuJPh..48..143S | 2214 | 69 | Radio sources observed with the Culgoora circular array. | SLEE O.B. | |||||
2000A&A...363..141R | 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 | 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. | ||
2021A&A...655A..17S | 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. |