CFHQS J022743-060530 , the SIMBAD biblio

CFHQS J022743-060530 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.06.08CEST04:26:46


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Title First 3 Authors
2009AJ....137.3541W 323       D S   X         8 9 54 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 42           X         1 21 187 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 168912 373 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 16       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 16       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 16       D               1 60 33 The dust content of QSO hosts at high redshift. CALURA F., GILLI R., VIGNALI C., et al.
2015MNRAS.446.2523B 174           X         4 2 27 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 17 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 26 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 2 25 64 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.
2017ApJ...840...24E 140       D     X         4 35 30 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 17       D               1 93 6 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 17       D               2 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...866..159V 17       D               1 98 1 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 ~ 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.
2019ApJ...879..117K 17       D               1 52 ~ High star formation rates of low Eddington ratio quasars at z >= 6. KIM Y. and IM M.
2019MNRAS.490.2542P viz 17       D               1 2245 ~ Unveiling the weak radio quasar population at z≥4. PERGER K., FREY S., GABANYI K.E., et al.
2020ApJ...903...60I 17       D               1 39 ~ 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 90             C       1 27 ~ The discovery of a highly accreting, radio-loud quasar at z = 6.82. BANADOS E., MAZZUCCHELLI C., MOMJIAN E., et al.
2021ApJ...908..124L 986     A D S   X C       21 38 ~ Constraining the quasar radio-loud fraction at z ∼ 6 with deep radio observations. LIU Y., WANG R., MOMJIAN E., et al.

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2023.06.08-04:26:46

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