activity
20082023
most citedThe VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release

381 citations · 2.7k across the 35 of their papers we have counts for

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Showing astro-ph.COShow all

17 papers · 1 filter

astro-ph.CO2020★ 311 cited

Improved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR

F. G. Mertens, M. Mevius, L. V. E Koopmans +23

A new upper limit on the 21-cm signal power spectrum at a redshift of is presented, based on 141 hours of data obtained with the Low-Frequency Array (LOFAR). The an…

astro-ph.CO2020★ 13 cited

Predictions for the 21cm-galaxy cross-power spectrum observable with SKA and future galaxy surveys

Dijana Vrbanec, Benedetta Ciardi, Vibor Jelic +4

In this paper we use radiative transfer + N-body simulations to explore the feasibility of measurements of cross-correlations between the 21cm field observed by the Square Kilomete…

astro-ph.CO2017★ 50 cited

Recovering the HII region size statistics from 21-cm tomography

Koki Kakiichi, Suman Majumdar, Garrelt Mellema +7

We introduce a novel technique, called "granulometry", to characterize and recover the mean size and the size distribution of HII regions from 21-cm tomography. The technique is ea…

astro-ph.CO2015★ 21 cited

A Bayesian analysis of redshifted 21-cm HI signal and foregrounds: Simulations for LOFAR

Abhik Ghosh, L. V. E. Koopmans, Emma Chapman +1

Observations of the EoR with the 21-cm hyperfine emission of neutral hydrogen (HI) promise to open an entirely new window onto the formation of the first stars, galaxies and accret…

astro-ph.CO2015★ 161 cited

The Cosmic Dawn and Epoch of Reionization with the Square Kilometre Array

L. V. E. Koopmans, J. Pritchard, G. Mellema +42

Concerted effort is currently ongoing to open up the Epoch of Reionization (EoR) (15-6) for studies with IR and radio telescopes. Whereas IR detections have been made of sou…

astro-ph.CO2015★ 20 cited

Simulating the 21cm forest detectable with LOFAR and SKA in the spectra of high-z GRBs

B. Ciardi, S. Inoue, F. B. Abdalla +26

We investigate the feasibility of detecting 21cm absorption features in the afterglow spectra of high redshift long Gamma Ray Bursts (GRBs). This is done employing simulations of c…