SDSS J103418.65+203300.2 , the SIMBAD biblio

SDSS J103418.65+203300.2 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST09:07:42


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Title First 3 Authors
2009AJ....138.1925M 15       D               1 60 13 Radio-selected quasars in the Sloan digital sky survey. McGREER I.D., HELFAND D.J. and WHITE R.L.
2010AJ....139.2360S viz 80069 836 The Sloan Digital Sky Survey quasar catalog. V. Seventh data release. SCHNEIDER D.P., RICHARDS G.T., HALL P.B., et al.
2010ApJ...718..392P viz 15       D               3 3759 150 A definitive survey for Lyman limit systems at z ∼ 3.5 with the Sloan Digital Sky Survey. PROCHASKA J.X., O'MEARA J.M. and WORSECK G.
2011MNRAS.410..860A viz 15       D               1 86770 182 A strong redshift dependence of the broad absorption line quasar fraction. ALLEN J.T., HEWETT P.C., MADDOX N., et al.
2011ApJS..194...45S viz 15       D               1 105786 1138 A catalog of quasar properties from Sloan Digital Sky Survey data release 7. SHEN Y., RICHARDS G.T., STRAUSS M.A., et al.
2012ApJ...753..106M viz 15       D               1 89523 227 A description of quasar variability measured using repeated SDSS and POSS imaging. MacLEOD C.L., IVEZIC Z., SESAR B., et al.
2014A&A...563A..54P viz 16       D               1 168926 217 The Sloan Digital Sky Survey quasar catalog: tenth data release. PARIS I., PETITJEAN P., AUBOURG E., et al.
2014ApJ...795L..29Y 16       D               1 14 15 SDSS J013127.34-032100.1: a newly discovered radio-loud quasar at z = 5.18 with extremely high luminosity. YI W.-M., WANG F., WU X.-B., et al.
2014MNRAS.445.1745W viz 16       D               1 163 146 The Giant Gemini GMOS survey of zem > 4.4 quasars - I. Measuring the mean free path across cosmic time. WORSECK G., PROCHASKA J.X., O'MEARA J.M., et al.
2015MNRAS.452..217C viz 16       D               1 182 137 The neutral hydrogen cosmological mass density at z = 5. CRIGHTON N.H.M., MURPHY M.T., PROCHASKA J.X., et al.
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.
2017A&A...597A..79P viz 16       D               1 302147 367 The Sloan Digital Sky Survey Quasar Catalog: Twelfth data release. PARIS I., PETITJEAN P., ROSS N.P., et al.
2018A&A...613A..51P viz 16       D               1 525784 350 The Sloan Digital Sky Survey Quasar Catalog: Fourteenth data release. PARIS I., PETITJEAN P., AUBOURG E., et al.
2020ApJ...888...85F viz 17       D               1 145239 ~ Ghostly strong Lyα absorbers: tracers of gas flows in the close vicinity of quasars? FATHIVAVSARI H.
2020MNRAS.494..789R viz 17       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.
2020ApJS..249...17R viz 17       D               1 525797 112 Spectral properties of quasars from Sloan Digital Sky Survey data release 14: the catalog. RAKSHIT S., STALIN C.S. and KOTILAINEN J.
2020ApJS..250....8L viz 17       D               1 750060 219 The Sloan Digital Sky Survey quasar catalog: Sixteenth Data Release. LYKE B.W., HIGLEY A.N., McLANE J.N., et al.
2020A&A...641A..85S 230       D     X         6 25 ~ Observations by GMRT at 323 MHz of radio-loud quasars at z > 5. SHAO Y., WAGG J., WANG R., et al.
2021ApJ...909...80B 18       D               1 27 52 The discovery of a highly accreting, radio-loud quasar at z = 6.82. BANADOS E., MAZZUCCHELLI C., 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..258...18C viz 18       D               4 78042 8 The completed Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey: the damped Lyα systems catalog. CHABANIER S., ETOURNEAU T., LE GOFF J.-M., et al.
2022A&A...659A.159S 332       D     X         8 27 5 The radio spectral turnover of radio-loud quasars at z > 5. SHAO Y., WAGG J., WANG R., et al.

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