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| 4C 16.63 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:32:21 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1967AJ.....72..757D | 627 | 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. | |||||
| 1972AJ.....77..625W | 492 | 6 | Observations at 750, 1400, and 2700 MHz of radio sources in the Vermilion Observatory survey. | WEBBER J.C. and WILLIS A.G. | |||||
| 1975AJ.....80..335S | 1092 | 38 | Positions and flux densities of 1075 radio sources at 365 MHz. | SHARP J.R. and BASH F.N. | |||||
| 1976A&A....50...47I | 53 | 26 | Aperture synthesis radio observations of three filamentary nebulae. | ISRAEL F.P. and FELLI M. | |||||
| 1989AJ.....97.1721C | 150 | 2 | Observations of the galactic radio structure CTB 63 (G 47.5+6.0) | CASWELL J.L., LANDECKER T.L. and ROGER R.S. | |||||
|
2010A&A...511A..53V |
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. | ||
|
2014ApJS..212...15F |
15 | D | 1 | 24788 | 60 | A broadband polarization catalog of extragalactic radio sources. | FARNES J.S., GAENSLER B.M. and CARRETTI E. | ||
|
2020MNRAS.497.3097M |
16 | D | 1 | 212 | 11 | The complex large-scale magnetic fields in the first Galactic quadrant as revealed by the Faraday depth profile disparity. | MA Y.K., MAO S.A., ORDOG A., et al. | ||
|
2021A&A...655A..17S |
17 | D | 1 | 338578 | 3 | The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. | STEIN Y., VOLLMER B., BOCH T., et al. | ||
| 2025MNRAS.541..306M | 112 | D | F | 3 | 202 | ~ | A new window into the sub-parsec scale magnetic field in the Milky Way? Unveiling small-scale magneto-ionic structures with Faraday complexity. | MA Y.K., SETA A., McCLURE-GRIFFITHS N.M., et al. |