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| SDSS J223907.56+003022.6 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST02:04:24 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2013ApJ...768..105M 
|
54 | D | X | 2 | 106 | 188 | The z = 5 quasar luminosity function from SDSS stripe 82. | McGREER I.D., JIANG L., FAN X., et al. | |
|
2016ApJ...819...24W
|
16 | D | 1 | 796 | 79 | A survey of luminous high-redshift quasars with SDSS and WISE. I. Target selection and optical spectroscopy. | WANG F., WU X.-B., FAN X., et al. | ||
|
2020MNRAS.494..789R
|
16 | D | 1 | 489 | 25 | The near and mid-infrared photometric properties of known redshift z >= 5 quasars. | ROSS N.P. and CROSS N.J.G. | ||
| 2020A&A...641A..85S | 263 | D | X | 7 | 25 | ~ | Observations by GMRT at 323 MHz of radio-loud quasars at z > 5. | SHAO Y., WAGG J., WANG R., 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.508.1853B | 17 | D | 1 | 83 | 68 | The mean free path of ionizing photons at 5 < z < 6: evidence for rapid evolution near reionization. | BECKER G.D., D'ALOISIO A., CHRISTENSON H.M., et al. | ||
|
2021A&A...656A.137G
|
17 | D | 1 | 493 | 12 | Low frequency radio properties of the z > 5 quasar population. | GLOUDEMANS A.J., DUNCAN K.J., ROTTGERING H.J.A., et al. | ||
| 2023ApJ...955..115Z | 17 | D | 1 | 99 | ~ | Probing Ultralate Reionization: Direct Measurements of the Mean Free Path over 5 < z < 6. | ZHU Y., BECKER G.D., CHRISTENSON H.M., et al. | ||
|
2024A&A...690A.321K
|
18 | D | X * | 7 | 59 | ~ | Revealing faint compact radio jets at redshifts above 5 with very long baseline interferometry. | KREZINGER M., BALDINI G., GIROLETTI M., et al. |
