Renyue Cen
educated at: Princeton University
occupation: researcher
official website: www.astro.princeton.edu/~cen
Articles 71
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Circumnuclear Molecular Gas in Low-redshift Quasars and Matched Star-forming Galaxies
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Observations of the missing baryons in the warm–hot intergalactic medium
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SCORCH. II. Radiation-hydrodynamic Simulations of Reionization with Varying Radiation Escape Fractions
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Long noncoding RNA HOXD-AS1 regulates proliferation of cervical cancer cells by activating Ras/ERK signaling pathway.
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The Most Ancient Spiral Galaxy: A 2.6-Gyr-old Disk with a Tranquil Velocity Field
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Probing the Dependence of the Intergalactic Medium on Large-scale Environment Using the Low-redshift Lyα Forest
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Testing the Large-scale Environments of Cool-core and Non-cool-core Clusters with Clustering Bias
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Large-scale clustering of Lyman α emission intensity from SDSS/BOSS
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Erratum: Towards simulating star formation in turbulent high-zgalaxies with mechanical supernova feedback
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What powers Lyαblobs?
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Do not forget the forest for the trees: the stellar-mass halo-mass relation in different environments
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Supernova feedback and the hot gas filling fraction of the interstellar medium
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Towards simulating star formation in turbulent high-z galaxies with mechanical supernova feedback
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The non-linear power spectrum of the Lyman alpha forest
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Gas loss in simulated galaxies as they fall into clusters
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Reionization on large scales. IV. Predictions for the 21 cm signal incorporating the light cone effect
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On the reversal of star formation rate-density relation at z = 1: insights from simulations
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ENZO: an adaptive mesh refinement code for astrophysics
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Shock waves and cosmic ray acceleration in the outskirts of galaxy clusters
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Chandra view of the warm-hot intergalactic medium toward 1ES 1553+113: absorption-line detections and identifications. I
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Alleviating the scaling problem of cosmological hydrodynamic simulations with HECA
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Multilocus sequence typing (MLST) analysis of 104 Clostridium difficile strains isolated from China.
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Comparisons of cosmological magnetohydrodynamic galaxy cluster simulations to radio observations
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Effects on galaxy evolution: pair interactions versus environment
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Probing the Very First Galaxies with the SKA
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Probing the first galaxies with the Square Kilometer Array
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Comparison of reionization models: radiative transfer simulations and approximate, seminumeric models
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EXTENDED Lyα EMISSION AROUND STAR-FORMING GALAXIES
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21cmfast: a fast, seminumerical simulation of the high-redshift 21-cm signal
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Radiative transfer modeling of Ly{alpha} emitters. II. New effects on galaxy clustering
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Radiative transfer modeling of Ly{alpha} emitters. I. Statistics of spectra and luminosity
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Galaxy size problem at z = 3: simulated galaxies are too small
Human - wd:Q62513709