CFHQS J022743-060530 , the SIMBAD biblio

CFHQS J022743-060530 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST02:46:28

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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
2009AJ....137.3541W 320       D S   X         8 9 103 Six more quasars at redshift 6 discovered by the Canada-France high-z quasar survey. WILLOTT C.J., DELORME P., REYLE C., et al.
2010AJ....140..546W 44           X         1 21 288 Eddington-limited accretion and the black hole mass function at redshift 6. WILLOTT C.J., ALBERT L., ARZOUMANIAN D., et al.
2010A&A...518A..10V viz 15       D               1 168913 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
2012RAA....12..865F 33 14 Observations of the first light and the epoch of reionization. FAN X.
2013A&A...552A..43O 15       D               1 20 18 The Canada-France High-z quasar Survey: 1.2mm observations. OMONT A., WILLOTT C.J., BEELEN A., et al.
2013ApJ...778..113B 15       D               1 18 17 WISE detections of known QSOs at redshifts greater than six. BLAIN A.W., ASSEF R., STERN D., et al.
2014MNRAS.438.2765C 15       D               1 60 42 The dust content of QSO hosts at high redshift. CALURA F., GILLI R., VIGNALI C., et al.
2015MNRAS.446.2523B 164           X         4 2 34 Combining Dark Energy Survey Science Verification data with near-infrared data from the ESO VISTA Hemisphere Survey. BANERJI M., JOUVEL S., LIN H., et al.
2016ApJ...816...85L 16       D               1 136 22 The contribution of host galaxies to the infrared energy output of z≳5.0 quasars. LYU J., RIEKE G.H. and ALBERTS S.
2016ApJ...819...24W viz 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.
2016ApJ...828...26M 3 25 167 Subaru high-z exploration of low-luminosity quasars (SHELLQs). I. Discovery of 15 quasars and bright galaxies at 5.7 < z < 6.9. MATSUOKA Y., ONOUE M., KASHIKAWA N., et al.
2016ApJS..227...11B viz 16       D               1 173 283 The Pan-STARRS1 distant z > 5.6 quasar survey: more than 100 quasars within the first Gyr of the Universe. BANADOS E., VENEMANS B.P., DECARLI R., et al.
2017ApJ...840...24E 136       D     X         4 35 121 Implications of z ∼ 6 quasar proximity zones for the epoch of reionization and quasar lifetimes. EILERS A.-C., DAVIES F.B., HENNAWI J.F., et al.
2018ApJS..237....5M 16       D               1 93 82 Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IV. Discovery of 41 quasars and luminous galaxies at 5.7 <= z <= 6.9. MATSUOKA Y., IWASAWA K., ONOUE M., et al.
2018ApJ...864...53E 18       D               2 49 104 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 98       D         F     2 60 137 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...866..159V 16       D               1 98 72 Dust emission in an accretion-rate-limited sample of z >= 6 quasars. VENEMANS B.P., DECARLI R., WALTER F., et al.
2018ApJ...869..150M 17       D               1 111 151 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 18       D               1 50 118 Gemini GNIRS near-infrared spectroscopy of 50 quasars at z >= 5.7. SHEN Y., WU J., JIANG L., et al.
2019ApJ...879..117K 16       D               1 52 ~ High star formation rates of low Eddington ratio quasars at z >= 6. KIM Y. and IM M.
2019MNRAS.490.2542P viz 16       D               1 2245 ~ Unveiling the weak radio quasar population at z≥4. PERGER K., FREY S., GABANYI K.E., et al.
2020MNRAS.494..789R viz 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.
2020ApJ...903...60I 16       D               1 39 13 Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XI. Proximity zone analysis for faint quasar spectra at z ∼ 6. ISHIMOTO R., KASHIKAWA N., ONOUE M., et al.
2021ApJ...909...80B 85             C       1 27 52 The discovery of a highly accreting, radio-loud quasar at z = 6.82. BANADOS E., MAZZUCCHELLI C., MOMJIAN E., et al.
2021ApJ...908..124L 920     A D S   X C       21 38 28 Constraining the quasar radio-loud fraction at z ∼ 6 with deep radio observations. LIU Y., WANG R., MOMJIAN E., et al.
2021A&A...656A.137G viz 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.
2022ApJS..259...20H viz 17       D               1 1042 83 GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10. HARIKANE Y., ONO Y., OUCHI M., et al.
2022ApJ...941..106F viz 17       D               1 120 26 The X-shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars. FARINA E.P., SCHINDLER J.-T., WALTER F., et al.
2023A&A...676A.115P 17       D               1 44 ~ Unraveling the formation histories of the first supermassive black holes with the Square Kilometre Array's pulsar timing array. PADMANABHAN H. and LOEB A.
2023ApJ...954..210A 17       D               1 14 ~ Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVIII. The Dark Matter Halo Mass of Quasars at z ∼ 6. ARITA J., KASHIKAWA N., MATSUOKA Y., et al.
2024MNRAS.528.5692K 45           X         1 17 ~ The radio-loud fraction of quasars at z > 6. KELLER P.M., THYAGARAJAN N., KUMAR A., et al.
2024A&A...690A.321K viz 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.

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