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| GB6 B1647+4608 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST12:24:08 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2019MNRAS.484..204C | 16 | D | 1 | 45 | 22 | The space density of z > 4 blazars. | CACCIANIGA A., MORETTI A., BELLADITTA S., et al. | ||
| 2019MNRAS.489.2732I | 16 | D | 3 | 25 | 24 | X-ray properties of z > 4 blazars. | IGHINA L., CACCIANIGA A., MORETTI A., et al. | ||
| 2019A&A...629A..68B | 81 | C | 2 | 12 | ~ | An extremely X-ray weak blazar at z = 5. | BELLADITTA S., MORETTI A., CACCIANIGA A., et al. | ||
| 2020A&A...635L...7B | 44 | X | 1 | 17 | 52 | The first blazar observed at z > 6. | BELLADITTA S., MORETTI A., CACCIANIGA A., et al. | ||
| 2021ApJ...909...80B | 18 | D | 1 | 27 | 52 | The discovery of a highly accreting, radio-loud quasar at z = 6.82. | BANADOS E., MAZZUCCHELLI C., MOMJIAN E., et al. | ||
| 2021MNRAS.503.4662M | 394 | D | X C | 9 | 4 | 7 | Flux-density measurements of the high-redshift blazar PSO J047.4478+27.2992 at 4.7 and 8.2 GHz with RATAN-600. | MUFAKHAROV T., MIKHAILOV A., SOTNIKOVA Y., et al. | |
2021MNRAS.508.2798S 
|
84 | X | 2 | 119 | 7 | High-redshift quasars at z >= 3 - I. Radio spectra. | SOTNIKOVA Y., MIKHAILOV A., MUFAKHAROV T., et al. | ||
|
2022MNRAS.511.5436D
|
17 | D | 1 | 19 | 10 | The evolution of the heaviest supermassive black holes in jetted AGNs. | DIANA A., CACCIANIGA A., IGHINA L., et al. | ||
|
2024A&A...690A.321K
|
18 | D | 1 | 59 | ~ | Revealing faint compact radio jets at redshifts above 5 with very long baseline interferometry. | KREZINGER M., BALDINI G., GIROLETTI M., et al. | ||
| 2026ApJS..282...21K | 420 | D | X | 9 | 23 | ~ | Milliarcsecond-resolution Radio-imaging Survey of Blazar Candidates at 4 < z < 5.4. | KREZINGER M., CACCIANIGA A., DALLACASA D., et al. |
