about
Signature of patchy reionization in the polarization anisotropy of the CMBInitial deep LOFAR observations of epoch of reionization windowsHalting type I planet migration in non-isothermal disksUpper Limits on the 21 cm Epoch of Reionization Power Spectrum from One Night with LOFAREffects of the sources of reionization on 21-cm redshift-space distortionsLinear polarization structures in LOFAR observations of the interstellar medium in the 3C 196 fieldLunar occultation of the diffuse radio sky: LOFAR measurements between 35 and 80 MHzSimulating the 21 cm forest detectable with LOFAR and SKA in the spectra of high-zGRBsInitial LOFAR observations of epoch of reionization windowsConstraining the epoch of reionization with the variance statistic: simulations of the LOFAR caseProbing reionization with LOFAR using 21-cm redshift space distortionsRecovering the H ii region size statistics from 21-cm tomographySimulating the impact of X-ray heating during the cosmic dawnThe effects of Lyman-limit systems on the evolution and observability of the epoch of reionizationPredictions for the 21 cm-galaxy cross-power spectrum observable with LOFAR and SubaruThe large-scale observational signatures of low-mass galaxies during reionizationEfficient photoheating algorithms in time-dependent photoionization simulationsThe wedge bias in reionization 21-cm power spectrum measurementsTurbulence in simulated H ii regionsStudying reionization with the next generation of Lyα emitter surveysOn the use of seminumerical simulations in predicting the 21-cm signal from the epoch of reionization2D GENUS TOPOLOGY OF 21-CM DIFFERENTIAL BRIGHTNESS TEMPERATURE DURING COSMIC REIONIZATIONLight cone effect on the reionization 21-cm signal – II. Evolution, anisotropies and observational implicationsSimulating cosmic reionization: how large a volume is large enough?Stars and reionization: the cross-correlation of the 21 cm line and the near-infrared backgroundLOFAR insights into the epoch of reionization from the cross-power spectrum of 21 cm emission and galaxiesOn the use of Lyα emitters as probes of reionizationProspects for detecting the 21 cm forest from the diffuse intergalactic medium with LOFARReionization and the Cosmic Dawn with the Square Kilometre ArrayThe brightness and spatial distributions of terrestrial radio sourcesThe inhomogeneous reionization of the local intergalactic medium by metal-poor globular clustersThe kinetic Sunyaev-Zel'dovich effect as a probe of the physics of cosmic reionization: the effect of self-regulated reionizationWill Nonlinear Peculiar Velocity and Inhomogeneous Reionization Spoil 21 cm Cosmology from the Epoch of Reionization?Imaging neutral hydrogen on large scales during the Epoch of Reionization with LOFARCan 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-examined
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description
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
G. Mellema
@nl
Garrelt Mellema
@en
Garrelt Mellema
@es
type
label
G. Mellema
@nl
Garrelt Mellema
@en
Garrelt Mellema
@es
altLabel
G. Mellema
@en
prefLabel
G. Mellema
@nl
Garrelt Mellema
@en
Garrelt Mellema
@es
P106
P1153
7004202562
P21
P31
P496
0000-0002-2512-6748