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QSO J1335+3533 , the SIMBAD biblio

QSO J1335+3533 , the SIMBAD biblio (49 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.06.03CEST22:40:23

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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
2006A&A...455..773V viz 108223 545 A catalogue of quasars and active nuclei: 12th edition. VERON-CETTY M.-P. and VERON P.
2006AJ....131.1203F 14 7 204 A survey of z>5.7 quasars in the Sloan Digital Sky Survey. IV. Discovery of seven additional quasars. FAN X., STRAUSS M.A., RICHARDS G.T., et al.
2006AJ....132..117F 24 19 939 Constraining the evolution of the ionizing background and the epoch of reionization with z∼6 quasars. II. A sample of 19 quasars. FAN X., STRAUSS M.A., BECKER R.H., et al.
2006ARA&A..44..415F 86             C       1 23 548 Observational constraints on cosmic reionization. FAN X., CARILLI C.L. and KEATING B.
2006MmSAI..77..635F 18 4 Evolution of high-redshift quasars. FAN X.
2006NewAR..50..665F 2 19 83 Evolution of high-redshift quasars. FAN X.-H.
2007AJ....134..617W 1 19 54 Millimeter and radio observations of z ∼ 6 quasars. WANG R., CARILLI C.L., BEELEN A., et al.
2008ApJ...687..848W 16       D               2 35 88 Thermal emission from warm dust in the most distant quasars. WANG R., CARILLI C.L., WAGG J., et al.
2009ApJ...696..580S viz 358       D     X C F     8 299 29 X-ray insights into the nature of weak emission-line quasars at high redshift. SHEMMER O., BRANDT W.N., ANDERSON S.F., et al.
2009ApJ...699..782D viz 76           X   F     1 5382 45 High-redshift SDSS quasars with weak emission lines. DIAMOND-STANIC A.M., FAN X., BRANDT W.N., et al.
2010ApJ...714..699W 288       D     X   F     7 18 162 Molecular gas in z ∼ 6 quasar host galaxies. WANG R., CARILLI C.L., NERI R., et al.
2010ApJ...714..834C 55       D     X         2 27 65 Ionization near zones associated with quasars at z ∼ 6. CARILLI C.L., WANG R., FAN X., 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.
2010A&A...522A..15M 172       D   O X C       4 11 84 Dust grain growth in the interstellar medium of 5 < z < 6.5 quasars. MICHALOWSKI M.J., MURPHY E.J., HJORTH J., et al.
2011ApJ...730..108R 15       D               1 49 34 Molecular gas in lensed z >2 quasar host galaxies and the star formation law for galaxies with luminous active galactic nuclei. RIECHERS D.A.
2011MNRAS.412.1926W 43           X         1 8 72 Near-zone sizes and the rest-frame extreme ultraviolet spectral index of the highest redshift quasars. WYITHE J.S.B. and BOLTON J.S.
2011ApJ...736...28W 39           X         1 34 54 A population of X-ray weak quasars: PHL 1811 analogs at high redshift. WU J., BRANDT W.N., HALL P.B., et al.
2011MNRAS.415.3237M 17       D               1 13 69 The first (nearly) model-independent constraint on the neutral hydrogen fraction at z ∼ 5-6. McGREER I.D., MESINGER A. and FAN X.
2011ApJ...743..163L 402       D     X C       10 42 17 The ultraviolet-to-mid-infrared spectral energy distribution of weak emission line quasars. LANE R.A., SHEMMER O., DIAMOND-STANIC A.M., et al.
2012MNRAS.423..774B 39           X         1 3 2 Joint Lyman α emitters – quasars reionization constraints. BAEK S., FERRARA A. and SEMELIN B.
2013MNRAS.428..226P viz 16       D               1 23 10 Finding new high-redshift quasars by asking the neighbours. POLSTERER K.L., ZINN P.-C. and GIESEKE F.
2013ApJ...772..103L 174       D     X   F     4 11 37 Complete infrared spectral energy distributions of millimeter detected quasars at z > 5. LEIPSKI C., MEISENHEIMER K., WALTER F., 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.
2014ApJ...785..154L 95       D       C       6 69 58 Spectral energy distributions of QSOs at z > 5: common active galactic nucleus-heated dust and occasionally strong star-formation. LEIPSKI C., MEISENHEIMER K., WALTER F., et al.
2014AJ....148...14B 16       D               2 44 80 Discovery of eight z ∼ 6 quasars from Pan-STARRS1. BANADOS E., VENEMANS B.P., MORGANSON E., et al.
2014MNRAS.444.2442V 17       D               1 17 38 High-redshift quasars host galaxies: is there a stellar mass crisis ? VALIANTE R., SCHNEIDER R., SALVADORI S., et al.
2015MNRAS.447..499M 21       D               1 23 134 Model-independent evidence in favour of an end to reionization by z ∼ 6. McGREER I.D., MESINGER A. and D'ODORICO V.
2015ApJ...804..118B 16       D               1 56 23 Constraining the radio-loud fraction of quasars at z > 5.5. BANADOS E., VENEMANS B.P., MORGANSON E., 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.
2016ARA&A..54..313M 83             C       1 25 64 The evolution of the intergalactic medium. McQUINN M.
2016ApJ...833..222J 58       D     X         2 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.
2017ApJ...840...24E 757       D S   X C       17 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.
2017A&A...603A.128N 140       D     X         4 30 14 The X-ray properties of z ∼ 6 luminous quasars. NANNI R., VIGNALI C., GILLI R., 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...867...30E 1673     A D S   X C       39 2 2 First spectroscopic study of a young quasar. EILERS A.-C., HENNAWI J.F. and DAVIES F.B.
2019ApJ...873...35S viz 17       D               2 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.
2019ApJ...883..163B viz 17       D               1 199 ~ The evolution of O I over 3.2 < z < 6.5: reionization of the circumgalactic medium. BECKER G.D., PETTINI M., RAFELSKI M., et al.
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 104       D     X         3 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.
2021AJ....161...45O viz 18       D               1 727 ~ The third data release of the KODIAQ survey. O'MEARA J.M., LEHNER N., HOWK J.C., et al.
2021ApJ...906...32Z 242       D     X C       5 31 ~ Strong Mg II and Fe II absorbers at 2.2 < z < 6.0. ZOU S., JIANG L., SHEN Y., et al.
2021ApJ...921...88M 108       D       C       2 18 ~ Estimating the effective lifetime of the z ∼ 6 quasar population from the composite proximity zone profile. MOREY K.A., EILERS A.-C., DAVIES F.B., et al.
2022MNRAS.514...55B 19       D               1 66 ~ Hydrogen reionization ends by z = 5.3: Lyman-α optical depth measured by the XQR-30 sample. BOSMAN S.E.I., DAVIES F.B., BECKER G.D., et al.
2022MNRAS.514.2855P 19       D               2 23 ~ Lensing in the darkness: a Bayesian analysis of 22 Chandra sources at z >= 6 shows no evidence of lensing. PACUCCI F., FOORD A., GORDON L., et al.
2023ApJ...942...59J 20       D               1 53 ~ (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.

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2023.06.03-22:40:23

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