QSO J0747+4434 , the SIMBAD biblio

QSO J0747+4434 , the SIMBAD biblio (58 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST22:13:59

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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
1999MNRAS.309L...1M 1 18 56 Submilimetre observations of luminous z - 4 radio-quiet quasars and the contribution of AGN to the submm source populations. McMAHON R.G., PRIDDEY R.S., OMONT A., et al.
2000AJ....119.1526S 42 71 Radio properties of z>4 optically selected quasars. STERN D., DJORGOVSKI S.G., PERLEY R.A., et al.
2000ESOSR..19....1V viz 180 ~ Quasars and Active Galactic Nuclei (9th Ed.). VERON-CETTY M.-P. and VERON P.
2001A&A...374..371O 70 164 A 1.2 mm MAMBO/IRAM-30 m survey of dust emission from the highest redshift PSS quasars. OMONT A., COX P., BERTOLDI F., et al.
2001AJ....121.1799P 33 91 Absorption systems in the spectra of 66 z≳4 quasars. PEROUX C., STORRIE-LOMBARDI L.J., McMAHON R.G., et al.
2001AJ....121.2843B viz 6250 77 Quasars in the 2MASS second incremental data release. BARKHOUSE W.A. and HALL P.B.
2002MNRAS.329..149I 68 91 The SCUBA Bright Quasar Survey (SBQS): 850-µm observations of the z ≳ 4 sample. ISAAK K.G., PRIDDEY R.S., McMAHON R.G., et al.
2002PASA...19..455C viz 237 30 A catalogue of damped Lyman alpha absorption systems and radio flux densities of the background quasars. CURRAN S.J., WEBB J.K., MURPHY M.T., et al.
2003A&A...412..707R viz 829 11 A catalogue of absorption-line systems in QSO spectra. RYABINKOV A.I., KAMINKER A.D. and VARSHALOVICH D.A.
2003MNRAS.346.1103P viz 676 238 The evolution of ΩHIand the epoch of formation of damped Lyman α absorbers. PEROUX C., McMAHON R.G., STORRIE-LOMBARDI L.J., et al.
2004A&A...417..443P 29 1 CIV absorbers in z >4 quasars: Tracing early galactic halos evolution. PEROUX C., PETITJEAN P., ARACIL B., et al.
2004AJ....127.2598S 1 51 191 The evolution of the intergalactic medium transmission to redshift 6. SONGAILA A.
2005AJ....129.2519V 24 70 X-ray lighthouses of the high-redshift universe. II. Further snapshot observations of the most luminous z≳4 quasars with Chandra. VIGNALI C., BRANDT W.N., SCHNEIDER D.P., et al.
2005AJ....130.1996S 26 54 The properties of intergalactic C IV and Si IV absorption. I. Optimal analysis of an extremely high signal-to-noise quasar sample. SONGAILA A.
2006A&A...455..773V viz 108224 628 A catalogue of quasars and active nuclei: 12th edition. VERON-CETTY M.-P. and VERON P.
2007AJ....133.2222S viz 5884 328 Clustering of high-redshift (z ≥ 2.9) quasars from the Sloan Digital Sky Survey. SHEN Y., STRAUSS M.A., OGURI M., et al.
2007MNRAS.377..657G 15       D               1 45 42 Evidence for overdensity around zem> 4 quasars from the proximity effect. GUIMARAES R., PETITJEAN P., ROLLINDE E., et al.
2007AJ....134..102S viz 77435 419 The Sloan Digital Sky Survey quasar catalog. IV. Fifth data release. SCHNEIDER D.P., HALL P.B., RICHARDS G.T., et al.
2007ApJ...665.1004J 2 61 301 The X-ray properties of the most luminous quasars from the Sloan Digital Sky Survey. JUST D.W., BRANDT W.N., SHEMMER O., et al.
2008ApJ...675.1002P viz 15       D               1 10397 50 The SDSS-DR5 survey for proximate damped Lyα systems. PROCHASKA J.X., HENNAWI J.F. and HERBERT-FORT S.
2008ApJ...680..169S viz 15       D               1 77431 447 Biases in virial black hole masses: an SDSS perspective. SHEN Y., GREENE J.E., STRAUSS M.A., et al.
2009ApJ...690..644G viz 15       D               1 1491 54 A full year's Chandra exposure on Sloan Digital Sky Survey quasars from the Chandra multiwavelength project. GREEN P.J., ALDCROFT T.L., RICHARDS G.T., et al.
2009ApJ...699..782D viz 15       D               1 5382 124 High-redshift SDSS quasars with weak emission lines. DIAMOND-STANIC A.M., FAN X., BRANDT W.N., et al.
2009ApJ...702..767W viz 15       D               1 280 29 Probing the origins of the CIV and FeKα Baldwin effects. WU J., VANDEN BERK D.E., BRANDT W.N., et al.
2009A&A...505..385A viz 15       D               1 99836 35 The large quasar reference frame (LQRF). An optical representation of the ICRS. ANDREI A.H., SOUCHAY J., ZACHARIAS N., et al.
2009A&A...505.1087N viz 15       D               1 1276 272 Evolution of the cosmological mass density of neutral gas from Sloan Digital Sky Survey II - Data Release 7. NOTERDAEME P., PETITJEAN P., LEDOUX C., et al.
2009A&A...508..133G viz 167       D S     C       5 99 19 Damped and sub-damped Lyman-α absorbers in z > 4 QSOs. GUIMARAES R., PETITJEAN P., DE CARVALHO R.R., et al.
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.
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.
2010ApJ...721.1448S 54       D     X         2 89 190 The evolution of Lyman limit absorption systems to redshift six. SONGAILA A. and COWIE L.L.
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...755...89R viz 15       D               3 216 300 Metallicity evolution of damped Lyα systems out to z ∼ 5. RAFELSKI M., WOLFE A.M., PROCHASKA J.X., et al.
2013ApJ...763...37C viz 16       D               1 26168 58 Precious metals in SDSS quasar spectra. I. Tracking the evolution of strong, 1.5 < z < 4.5 C IV absorbers with thousands of systems. COOKSEY K.L., KAO M.M., SIMCOE R.A., et al.
2013MNRAS.430.2680M 17       D               1 34 89 Mass-metallicity relation from z = 5 to the present: evidence for a transition in the mode of galaxy growth at z = 2.6 due to the end of sustained primordial gas infall. MOLLER P., FYNBO J.P.U., LEDOUX C., et al.
2013ApJS..206....4K viz 16       D               1 119612 109 Mean spectral energy distributions and bolometric corrections for luminous quasars. KRAWCZYK C.M., RICHARDS G.T., MEHTA S.S., et al.
2013ApJ...769...54N viz 16       D               2 86 101 The fundamental plane of damped Lyα systems. NEELEMAN M., WOLFE A.M., PROCHASKA J.X., et al.
2013ApJ...775..119C 16       D               2 23 1 A mini X-ray survey of sub-damped lyman-alpha absorption systems: searching for active galactic nuclei formed in protogalaxies. CHARTAS G., KULKARNI V.P. and ASPER A.
2013ApJ...779..161S viz 16       D               1 79596 24 Precious metals in SDSS quasar spectra. II. Tracking the evolution of strong, 0.4 < z < 2.3 Mg II absorbers with thousands of systems. SEYFFERT E.N., COOKSEY K.L., SIMCOE R.A., 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.
2014ApJS..215...12C viz 16       D               1 9705 7 Catalog of narrow C IV absorption lines in BOSS. II. For quasars with zem> 2.4. CHEN Z.-F., QIN Y.-P., QIN M., et al.
2015AJ....150..111O viz 16       D               2 171 71 The first data release of the KODIAQ survey. O'MEARA J.M., LEHNER N., HOWK J.C., et al.
2015MNRAS.452.4326B viz 16       D               1 328 26 The chemistry of the most metal-rich damped Lyman α systems at z ∼ 2 - II. Context with the Local Group. BERG T.A.M., ELLISON S.L., PROCHASKA J.X., et al.
2015ApJ...815...33R viz 16       D               1 814 170 A Hubble diagram for quasars. RISALITI G. and LUSSO E.
2016MNRAS.458.4074Q viz 16       D               1 368 72 The ESO UVES advanced data products quasar sample - VI. Sub-damped Lyman α metallicity measurements and the circumgalactic medium. QUIRET S., PEROUX C., ZAFAR T., et al.
2016MNRAS.462.2980C viz 16       D               1 23508 1 Narrow C IV absorption doublets on quasar spectra of the Baryon Oscillation Spectroscopic Survey. CHEN Z.-F., GU Q.-S., ZHOU L., 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.
2017AJ....154..114O viz 16       D               1 298 26 The second data release of the KODIAQ survey. O'MEARA J.M., LEHNER N., HOWK J.C., et al.
2018A&A...613A..51P viz 16       D               2 525784 350 The Sloan Digital Sky Survey Quasar Catalog: Fourteenth data release. PARIS I., PETITJEAN P., AUBOURG E., et al.
2019A&A...631A.120S 84             C       1 53 ~ Quasars as standard candles II. The non-linear relation between UV and X-ray emission at high redshifts. SALVESTRINI F., RISALITI G., BISOGNI S., 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...888...85F viz 17       D               1 145239 ~ Ghostly strong Lyα absorbers: tracers of gas flows in the close vicinity of quasars? FATHIVAVSARI H.
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...642A.150L viz 17       D               1 2429 92 Quasars as standard candles. III. Validation of a new sample for cosmological studies. LUSSO E., RISALITI G., NARDINI E., et al.
2021AJ....161...45O viz 17       D               4 727 ~ The third data release of the KODIAQ survey. O'MEARA J.M., LEHNER N., HOWK J.C., et al.
2022ApJS..258...18C viz 18       D               2 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.

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