Standout Papers

Enriched haloes at redshift z = 2 with no star formation: implications for accretion and wind sce... 2011 2026 2016 2021 46
  1. Enriched haloes at redshift z = 2 with no star formation: implications for accretion and wind scenarios★ (2011)
    N. Bouché, M. T. Murphy et al. Monthly Notices of the Royal Astronomical Society

Citation Impact

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The ESO UVES advanced data products quasar sample
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Investigating lensing by absorbers in the 2dF-quasar survey
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The ESO UVES Advanced Data Products Quasar Sample - II. Cosmological Evolution of the Neutral Gas Mass Density
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X-shooter UV- to K-band intermediate-resolution high-efficiency spectrograph for the VLT: status report at the final design review
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Metal-rich damped/subdamped Lyman   quasar absorbers at z < 1
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Classical and Mg ii-selected damped Lyman α absorbers: impact on ΩH iatz< 1.7
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THE VLT SINFONI Mg ii PROGRAM FOR LINE EMITTERS (SIMPLE). II. BACKGROUND QUASARS PROBING $Z\sim 1$ GALACTIC WINDS
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A homogeneous sample of sub-damped Lyman   systems -- III. Total gas mass ohmH I+He II at z > 2
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The SINFONI Mg ii Program for Line Emitters (SIMPLE): Discovering Starbursts near QSO Sight Lines
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The missing metals problem - III. How many metals are expelled from galaxies?
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A homogeneous sample of sub-damped Lyman alpha systems - I. Construction of the sample and chemical abundance measurements
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A homogeneous sample of sub-damped Lyman alpha systems - II. Statistical, kinematic and chemical properties
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A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems
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The evolution of ΩH iand the epoch of formation of damped Lyman α absorbers
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The SCUBA Bright Quasar Survey (SBQS): 850-μm observations of thez≳ 4 sample
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The most metal-rich intervening quasar absorber known
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The missing metals problem – II. How many metals are in z ⋍ 2.2 galaxies?
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A MIKE + UVES survey of sub-damped Lyman α systems atz< 1.5
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