Renyue Cen researcher
Cen, Renyue
VIAF ID: 31848864 (Personal)
Permalink: http://viaf.org/viaf/31848864
Preferred Forms
- 100 1 _ ‡a Cen, Renyue
- 100 1 0 ‡a Cen, Renyue
- 100 1 _ ‡a Cen, Renyue
- 100 0 _ ‡a Renyue Cen ‡c researcher
4xx's: Alternate Name Forms (1)
Works
Title | Sources |
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21cmfast: a fast, seminumerical simulation of the high-redshift 21-cm signal | |
Alleviating the scaling problem of cosmological hydrodynamic simulations with HECA | |
Background X-Ray Emission from Hot Gas in CDM and CDM+ Lambda Universes: Spectral Signatures | |
Can standard cosmological models explain the observed Abell cluster bulk flow? | |
Chandra view of the warm-hot intergalactic medium toward 1ES 1553+113: absorption-line detections and identifications. I | |
Circumnuclear Molecular Gas in Low-redshift Quasars and Matched Star-forming Galaxies | |
Comparison of reionization models: radiative transfer simulations and approximate, seminumeric models | |
Constraining Ω with Cluster Evolution | |
A Constraint on the Gravitational Lensing Magnification and Age of the Redshiftz = 6.28 Quasar SDSS 1030+0524 | |
Cosmic Reionization and the 21 cm Signal: Comparison between an Analytical Model and a Simulation | |
A cosmological hydrodynamic code based on the total variation diminishing scheme | |
Cosmological Mestel Disks and the Rossby Vortex Instability: The Origin of Supermassive Black Holes | |
Detecting X-ray filaments in the low-redshift Universe with XEUS and Constellation-X | |
Determining the Amplitude of Mass Fluctuations in the Universe | |
Do not forget the forest for the trees: the stellar-mass halo-mass relation in different environments | |
Effects on galaxy evolution: pair interactions versus environment | |
ENZO: an adaptive mesh refinement code for astrophysics | |
Evolution of Lyman break galaxies beyond z = 4 | |
EXTENDED Lyα EMISSION AROUND STAR-FORMING GALAXIES | |
Galaxy size problem at z = 3: simulated galaxies are too small | |
Gas loss in simulated galaxies as they fall into clusters | |
A hydrodynamic approach to cosmology: The mixed dark matter cosmological scenario | |
Hydrodynamic Simulations of the Lyman Alpha Forest in a Theory of Gravitational Collapse | |
Implications of the Lyα Emission Line from a Candidate z = 10 Galaxy | |
Is There a Missing Galaxy Problem at High Redshift? | |
Large-scale clustering of Lyman α emission intensity from SDSS/BOSS | |
The Local Group as a test of cosmological models | |
Long noncoding RNA HOXD-AS1 regulates proliferation of cervical cancer cells by activating Ras/ERK signaling pathway | |
The Lyα Forest Power Spectrum from the Sloan Digital Sky Survey | |
Massive Galaxies in Cosmological Simulations: Ultraviolet‐selected Sample at Redshiftz = 2 | |
The Metal Enrichment and Temperature of the Intergalactic Medium | |
The Most Ancient Spiral Galaxy: A 2.6-Gyr-old Disk with a Tranquil Velocity Field | |
Multilocus sequence typing (MLST) analysis of 104 Clostridium difficile strains isolated from China. | |
The non-linear power spectrum of the Lyman alpha forest | |
On the reversal of star formation rate-density relation at z = 1: insights from simulations | |
A piecewise parabolic method for cosmological hydrodynamics | |
Probing the Dependence of the Intergalactic Medium on Large-scale Environment Using the Low-redshift Lyα Forest | |
Probing the first galaxies with the Square Kilometer Array | |
Probing the Reionization History Using the Spectra of High‐Redshift Sources | |
Proposed SMEX to spectrally analyze the diffuse x-ray background: The Baryonic Extragalactic Structure Tracer (BEST) | |
The Protogalactic Origin for Cosmic Magnetic Fields | |
Radiative transfer modeling of Ly{alpha} emitters. II. New effects on galaxy clustering | |
Reionization on large scales. IV. Predictions for the 21 cm signal incorporating the light cone effect | |
The relationship between dietary factors and serum lipids in southern Chinese population samples | |
The Santa Barbara Cluster Comparison Project: A Comparison of Cosmological Hydrodynamics Solutions | |
SCORCH. II. Radiation-hydrodynamic Simulations of Reionization with Varying Radiation Escape Fractions | |
Shock‐heated Gas in the Large‐Scale Structure of the Universe | |
Shock waves and cosmic ray acceleration in the outskirts of galaxy clusters | |
Supernova feedback and the hot gas filling fraction of the interstellar medium | |
Testing cosmogonic models with gravitational lensing | |
Testing the Large-scale Environments of Cool-core and Non-cool-core Clusters with Clustering Bias | |
Towards simulating star formation in turbulent high-z galaxies with mechanical supernova feedback | |
Tracing early structure formation with massive starburst galaxies and their implications for reionization | |
Tracing the warm-hot intergalactic medium in the local Universe | |
What powers Lyαblobs? | |
X-ray clusters from a high-resolution hydrodynamic PPM simulation of the cold dark matter universe |