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QSO J0810+5105 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.03.23CET22:10:38 |
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 |
---|---|---|---|---|---|---|---|---|---|
2016ApJ...833..222J | 180 | D | X | 5 | 52 | 64 | The final SDSS high-redshift quasar sample of 52 quasars at z>5.7. | JIANG L., McGREER I.D., FAN X., et al. | |
2018ApJ...864...53E | 42 | X | 1 | 49 | 6 | The opacity of the intergalactic medium measured along quasar sightlines at z ∼ 6. | EILERS A.-C., DAVIES F.B. and HENNAWI J.F. | ||
2018MNRAS.479.1055B | 100 | D | F | 2 | 60 | 14 | New constraints on Lyman-α opacity with a sample of 62 quasars at z > 5.7. | BOSMAN S.E.I., FAN X., JIANG L., et al. | |
2018ApJ...869..150M | 17 | D | 1 | 111 | ~ | Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). V. Quasar luminosity function and contribution to cosmic reionization at z = 6. | MATSUOKA Y., STRAUSS M.A., KASHIKAWA N., et al. | ||
2019ApJ...873...35S ![]() |
17 | D | 1 | 50 | ~ | Gemini GNIRS near-infrared spectroscopy of 50 quasars at z >= 5.7. | SHEN Y., WU J., JIANG L., et al. | ||
2020ApJ...900...12L | 17 | D | 5 | 53 | ~ | SCUBA2 High rEdshift bRight quasaR surveY: far-infrared properties and weak-line features. | LI Q., WANG R., FAN X., et al. | ||
2021ApJ...906...32Z | 18 | D | 1 | 31 | ~ | Strong Mg II and Fe II absorbers at 2.2 < z < 6.0. | ZOU S., JIANG L., SHEN Y., et al. | ||
2021A&A...656A.137G ![]() |
18 | D | 1 | 17 | ~ | Low frequency radio properties of the z > 5 quasar population. | GLOUDEMANS A.J., DUNCAN K.J., ROTTGERING H.J.A., et al. | ||
2022ApJ...925..121W | 19 | D | 2 | 34 | ~ | Metallicity in Quasar Broad-line Regions at Redshift ∼ 6. | WANG S., JIANG L., SHEN Y., et al. | ||
2023ApJ...944..159F | 20 | D | 1 | 168 | ~ | 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. |
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