QSO J0334-1612 , the SIMBAD biblio

QSO J0334-1612 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST02:31:43


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Title First 3 Authors
2000ApJ...543..552S viz 636 252 Surveys for z>3 damped Lyα absorption systems: the evolution of neutral gas. STORRIE-LOMBARDI L.J. and WOLFE A.M.
2001MNRAS.322..933S 34 19 The Second APM UKST Colour Survey for z>4 quasars. STORRIE-LOMBARDI L.J., IRWIN M.J., 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.
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.
2005MNRAS.363..479P 2 17 126 A homogeneous sample of sub-damped Lyman α systems - III. Total gas mass ΩHI+HeIIat z > 2. PEROUX C., DESSAUGES-ZAVADSKY M., D'ODORICO S., et al.
2006A&A...455..773V viz 108223 628 A catalogue of quasars and active nuclei: 12th edition. VERON-CETTY M.-P. and VERON P.
2007ApJ...665.1004J 1 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.
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 16       D               1 88 190 The evolution of Lyman limit absorption systems to redshift six. SONGAILA A. and COWIE L.L.
2012ApJ...761..112M viz 15       D               5 47 42 A survey of Mg II absorption at 2 < z < 6 with Magellan/FIRE. I. Sample and evolution of the Mg II frequency. MATEJEK M.S. and SIMCOE R.A.
2013ApJ...764....9M viz 15       D               20 231 12 Mg II absorption at 2 < z < 6 with Magellan/FIRE. II. A longitudinal study of H I, metals, and ionization in galactic halos. MATEJEK M.S., SIMCOE R.A., COOKSEY K.L., et al.
2014MNRAS.444..744Z viz 39           X         1 24 21 The ESO UVES advanced data products quasar sample - III. Evidence of bimodality in the [N/α] distribution. ZAFAR T., CENTURION M., PEROUX C., et al.
2015ApJ...815...33R viz 16       D               1 814 170 A Hubble diagram for quasars. RISALITI G. and LUSSO E.
2016MNRAS.456.4488S viz 16       D               2 63 62 The evolution of neutral gas in damped Lyman α systems from the XQ-100 survey. SANCHEZ-RAMIREZ R., ELLISON S.L., PROCHASKA J.X., et al.
2019MNRAS.482.3458M viz 16       D               1 472 60 The UVES Spectral Quasar Absorption Database (SQUAD) data release 1: the first 10 million seconds. MURPHY M.T., KACPRZAK G.G., SAVORGNAN G.A.D., et al.
2020MNRAS.491.2057L viz 16       D               2 92 33 MUSE Analysis of Gas around Galaxies (MAGG) - I: Survey design and the environment of a near pristine gas cloud at z ≃ 3.5. LOFTHOUSE E.K., FUMAGALLI M., FOSSATI M., et al.
2021AJ....161...45O viz 17       D               2 727 ~ The third data release of the KODIAQ survey. O'MEARA J.M., LEHNER N., HOWK J.C., et al.
2021MNRAS.503.3044F 85               F     1 30 32 MUSE analysis of gas around galaxies (MAGG) - III. The gas and galaxy environment of z = 3-4.5 quasars. FOSSATI M., FUMAGALLI M., LOFTHOUSE E.K., et al.
2023MNRAS.518..305L 17       D               1 30 13 MUSE Analysis of Gas around Galaxies (MAGG) - IV. The gaseous environment of z ∼ 3-4 Ly α emitting galaxies. LOFTHOUSE E.K., FUMAGALLI M., FOSSATI M., et al.

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