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| QSO J0910+1656 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST18:08:31 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2019ApJ...884...30W | 229 | D | X | 6 | 34 | 128 | Exploring reionization-era quasars. III. Discovery of 16 quasars at 6.4 <= z <= 6.9 with DESI Legacy imaging Surveys and the UKIRT Hemisphere Survey and quasar luminosity function at z ∼ 6.7. | WANG F., YANG J., FAN X., et al. | |
2019MNRAS.490.2542P 
|
17 | D | 1 | 2245 | ~ | Unveiling the weak radio quasar population at z≥4. | PERGER K., FREY S., GABANYI K.E., et al. | ||
|
2020MNRAS.494..789R
|
17 | 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. | ||
| 2020ApJ...904...26Y | 19 | D | 4 | 32 | 67 | Measurements of the z ∼ 6 intergalactic medium optical depth and transmission spikes using a new z > 6.3 quasar sample. | YANG J., WANG F., FAN X., 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. | ||
| 2022MNRAS.513.1801L | 18 | D | 1 | 27 | 14 | Chemical abundance of z ∼ 6 quasar broad-line regions in the XQR-30 sample. | LAI S., BIAN F., ONKEN C.A., et al. | ||
| 2023ApJ...942...59J | 19 | D | 1 | 53 | 7 | (Nearly) Model-independent Constraints on the Neutral Hydrogen Fraction in the Intergalactic Medium at z ∼ 5-7 Using Dark Pixel Fractions in Lyα and Lyβ Forests. | JIN X., YANG J., FAN X., et al. | ||
| 2023ApJ...944..159F | 19 | D | 1 | 168 | 2 | In Situ Star Formation in Accretion Disks and Explanation of Correlation between the Black Hole Mass and Metallicity in Active Galactic Nuclei. | FAN X. and WU Q. |
