QSO J0810+5105 , the SIMBAD biblio

QSO J0810+5105 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.03.23CET22:10:38


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Bibcode/DOI Score in Title|Abstract|
Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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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 viz 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 viz 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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2023.03.23-22:10:38

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