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| 4C 04.68 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:38:45 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1975AJ.....80..335S | 1092 | 38 | Positions and flux densities of 1075 radio sources at 365 MHz. | SHARP J.R. and BASH F.N. | |||||
| 1986A&A...163...77B | 6 | 4 | Detection of a nuclear coherent radiation component in the 408 MHz radio emission of SS 433. | BONSIGNORI-FACONDI S.R. and BRACCESI A. | |||||
| 1986A&A...166..157B | 6 | 14 | Quiescent and active flaring periods in SS 433 at 408 MHz. | BONSIGNORI-FACONDI S.R., PADRIELLI L., MONTEBUGNOLI S., et al. | |||||
| 1988SoSAO..58...41A | 795 | 4 | A deep sky survey at 3.9, 7.7 and 14.4 GHz. | AMIRKHANIAN V.R., GORSHKOV A.G. and IPATOV A.V. | |||||
| 1993A&A...270..189V | 18 | 12 | Daily spectra of radio flares from SS 433 in May/June 1987. | VERMEULEN R.C., McADAM W.B., TRUSHKIN S.A., et al. | |||||
|
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. | ||
|
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. | ||
|
2022ApJS..260....4P |
17 | D | 1 | 7976 | 3 | Direction of Parsec-scale Jets for 9220 Active Galactic Nuclei. | PLAVIN A.V., KOVALEV Y.Y. and PUSHKAREV A.B. | ||
| 2025MNRAS.541..306M | 112 | D | F | 2 | 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. |