about
Signature of patchy reionization in the polarization anisotropy of the CMBThe HiiRegion of the First StarProbing reionization with LOFAR using 21-cm redshift space distortionsLikely Values of the Cosmological ConstantThe effects of Lyman-limit systems on the evolution and observability of the epoch of reionizationThe large-scale observational signatures of low-mass galaxies during reionizationLight cone effect on the reionization 21-cm signal – II. Evolution, anisotropies and observational implicationsSimulating cosmic reionization: how large a volume is large enough?On the use of Lyα emitters as probes of reionizationThe kinetic Sunyaev-Zel'dovich effect as a probe of the physics of cosmic reionization: the effect of self-regulated reionizationCan 21-cm observations discriminate between high-mass and low-mass galaxies as reionization sources?Detecting the rise and fall of the first stars by their impact on cosmic reionizationLight-cone effect on the reionization 21-cm power spectrumProspects of observing a quasar H ii region during the epoch of reionization with the redshifted 21-cm signalRadiative transfer of energetic photons: X-rays and helium ionization in C2-RayRedshift-space distortion of the 21-cm background from the epoch of reionization - I. Methodology re-examinedSimulating cosmic reionization and the radiation backgrounds from the epoch of reionizationErratum: Observational constraints on supermassive dark starsTopology and sizes of H ii regions during cosmic reionizationCosmological Reionization by the First Stars in the H[sub 2]-Dissociating BackgroundMeasuring the history of cosmic reionization using the 21-cm probability distribution function from simulationsObservational constraints on supermassive dark starsThe inhomogeneous background of H_2_-Dissociating radiation during cosmic reionizationCosmological radiative transfer comparison project â II. The radiation-hydrodynamic testsReionization: characteristic scales, topology and observabilityCurrent models of the observable consequences of cosmic reionization and their detectabilitySimulating Reionization: Character and ObservabilityThe effect of the intergalactic environment on the observability of Lyα emitters during reionizationThe Inhomogeneous Background of H2 Dissociating Radiation During Cosmic ReionizationThe Theory and Simulation of the 21‐cm Background from the Epoch of ReionizationSelf-regulated reionizationThe Kinetic Sunyaev‐Zel’dovich Effect from Radiative Transfer Simulations of Patchy ReionizationC2-ray: A new method for photon-conserving transport of ionizing radiationCosmological radiative transfer codes comparison project ��� I. The static density field testsDynamical HiiRegion Evolution in Turbulent Molecular CloudsSimulating cosmic reionization at large scales - I. The geometry of reionizationSimulating cosmic reionization at large scales - II. The 21-cm emission features and statistical signalskSZ from patchy reionization: The view from the simulationsIonisation fronts and their interaction with density fluctuations: implications for reionisationFragmentation and Evolution of Molecular Clouds. I. Algorithm and First Results
P50
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P50
description
Amerikaans astrofysicus
@nl
astrophysicien américain
@fr
name
Paul Shapiro
@ast
Paul Shapiro
@es
Paul Shapiro
@fr
Paul Shapiro
@nl
type
label
Paul Shapiro
@ast
Paul Shapiro
@es
Paul Shapiro
@fr
Paul Shapiro
@nl
altLabel
Paul R. Shapiro
@fr
Paul Robert Shapiro
@fr
prefLabel
Paul Shapiro
@ast
Paul Shapiro
@es
Paul Shapiro
@fr
Paul Shapiro
@nl