activity
20042025
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 5.8k across the 39 of their papers we have counts for

collaborators

40 papers

astro-ph.GA2025★ 2 cited

The MeerKAT Fornax Survey V. H i kinematics and Fornax cluster membership of the dwarf galaxy ESO 358-60

P. Kamphuis, P. Serra, D. Kleiner +2

The MeerKAT Fornax Survey (MFS) is a large survey project mapping the HI in the Fornax cluster. Most of the cluster members detected in HI show significant signs of interaction wit…

astro-ph.SR2024★ 17 cited

Exploring the time variability of the Solar Wind using LOFAR pulsar data

S. C. Susarla, A. Chalumeau, C. Tiburzi +22

High-precision pulsar timing is highly dependent on precise and accurate modeling of any effects that impact the data. It was shown that commonly used Solar Wind models do not accu…

astro-ph.GA2024★ 46 cited

MHONGOOSE -- A MeerKAT Nearby Galaxy HI Survey

W. J. G. de Blok, J. Healy, F. M. Maccagni +57

The MHONGOOSE (MeerKAT HI Observations of Nearby Galactic Objects: Observing Southern Emitters) survey maps the distribution and kinematics of the neutral atomic hydrogen (HI) gas…

astro-ph.GA2023★ 1 cited

The MeerKAT Fornax Survey -- I. Survey description and first evidence of ram pressure in the Fornax galaxy cluster

P. Serra, F. M. Maccagni, D. Kleiner +22

The MeerKAT Fornax Survey maps the distribution and kinematics of atomic neutral hydrogen gas (HI) in the nearby Fornax galaxy cluster using the MeerKAT telescope. The 12 deg^2 sur…

astro-ph.HE2022

The LOFAR Tied-Array All-Sky Survey: Timing of 35 radio pulsars and an overview of the properties of the LOFAR pulsar discoveries

E. van der Wateren, C. G. Bassa, S. Cooper +20

The LOFAR Tied-Array All-Sky Survey (LOTAAS) is the most sensitive untargeted radio pulsar survey performed at low radio frequencies (119--151\,MHz) to date and has discovered 76 n…

astro-ph.GA2022★ 16 cited

HALOGAS: Strong Constraints on the Neutral Gas Reservoir and Accretion Rate in Nearby Spiral Galaxies

P. Kamphuis, E. Jütte, G. H. Heald +11

Galaxies in the local Universe are thought to require ongoing replenishment of their gas reservoir in order to maintain the observed star formation rates. Cosmological simulations…

astro-ph.GA2022★ 6 cited

A depolarizing HI tidal tail in the western lobe of Fornax A

Francesca Loi, Paolo Serra, Matteo Murgia +8

Recent MeerKAT neutral hydrogen (HI) observations of Fornax A reveal tidal material intersecting in projection the western lobe of this radio galaxy. We found a spatial coincidence…

astro-ph.CO2021★ 8 cited

Faint polarised sources in the Lockman Hole field at 1.4 GHz

A. Berger, B. Adebahr, N. Herrera Ruiz +3

We aim to study the nature of the faint, polarised radio source population whose source composition and redshift dependence contain information about the strength, morphology, and…

astro-ph.HE2020★ 55 cited

The impact of Solar wind variability on pulsar timing

C. Tiburzi, G. M. Shaifullah, C. G. Bassa +22

High-precision pulsar timing requires accurate corrections for dispersive delays of radio waves, parametrized by the dispersion measure (DM), particularly if these delays are varia…

astro-ph.GA2020★ 6 cited

Hot gas heating via magnetic arms in spiral galaxies. The case of M 83

M. Wezgowiec, M. Ehle, M. Soida +3

Reconnection heating has been considered as a potential source of the heating of the interstellar medium. In some galaxies, significant polarised radio emission has been found betw…

astro-ph.GA2019★ 65 cited

HALOGAS: the properties of extraplanar HI in disc galaxies

A. Marasco, F. Fraternali, G. Heald +9

We present a systematic study of the extraplanar gas (EPG) in a sample of 15 nearby late-type galaxies at intermediate inclinations using publicly available, deep interferometric H…

astro-ph.HE2019★ 45 cited

On the usefulness of existing Solar-wind models for pulsar timing corrections

C. Tiburzi, J. P. W. Verbiest, G. M. Shaifullah +15

Dispersive delays due to the Solar wind introduce excess noise in high-precision pulsar timing experiments, and must be removed in order to achieve the accuracy needed to detect, e…

astro-ph.GA2018★ 6 cited

A star-forming dwarf galaxy candidate in the halo of NGC 4634

Y. Stein, D. J. Bomans, P. Kamphuis +3

The halos of disk galaxies form a crucial connection between the galaxy disk and the intergalactic medium. Massive stars, HII regions, or dwarf galaxies located in the halos of gal…

astro-ph.GA2018★ 39 cited

Investigation of the cosmic ray population and magnetic field strength in the halo of NGC 891

D. D. Mulcahy, A. Horneffer, R. Beck +24

Low-frequency radio continuum observations of edge-on galaxies are ideal to study cosmic-ray electrons (CREs) in halos via radio synchrotron emission and to measure magnetic field…

astro-ph.GA2018★ 11 cited

CHANG-ES XI: Circular Polarization in the Cores of Nearby Galaxies

Judith A Irwin, Richard N. Henriksen, Marek Wezgowiec +18

We detect 5 galaxies in the CHANG-ES (Continuum Halos in Nearby Galaxies -- an EVLA Survey) sample that show circular polarization (CP) at L-band in our high resolution data sets.…

astro-ph.GA2018★ 25 cited

Exploring the making of a galactic wind in the star-bursting dwarf irregular galaxy IC 10 with LOFAR

V. Heesen, D. A. Rafferty, A. Horneffer +16

Low-mass galaxies are subject to strong galactic outflows, in which cosmic rays may play an important role, they can be best traced with low-frequency radio continuum observations,…

astro-ph.GA2018★ 78 cited

Radio haloes in nearby galaxies modelled with 1D cosmic-ray transport using SPINNAKER

V. Heesen, M. Krause, R. Beck +10

We present radio continuum maps of 12 nearby (), edge-on (), late-type spiral galaxies mostly at and 5 GHz, observed with the Australia Te…

astro-ph.GA2017★ 29 cited

M82 - A radio continuum and polarisation study II. Polarisation and rotation measures

B. Adebahr, M. Krause, U. Klein +2

The composition and morphology of the interstellar medium in starburst galaxies has been well investigated, but the magnetic field properties are still uncertain. The nearby starbu…

astro-ph.GA2017

The MeerKAT Fornax Survey

P. Serra, W. J. G. de Blok, G. L. Bryan +18

We present the science case and observations plan of the MeerKAT Fornax Survey, an HI and radio continuum survey of the Fornax galaxy cluster to be carried out with the SKA precurs…

astro-ph.GA2017★ 30 cited

Star formation driven galactic winds in UGC 10043

C. López-Cobá, S. F. Sánchez, A. V. Moiseev +15

We study the galactic wind in the edge-on spiral galaxy UGC 10043 with the combination of the CALIFA integral field spectroscopy data, scanning Fabry-Perot interferometry (FPI), an…

astro-ph.GA2016★ 136 cited

Two-dimensional multi-component photometric decomposition of CALIFA galaxies

J. Mendez-Abreu, T. Ruiz-Lara, L. Sanchez-Menguiano +20

We present a two-dimensional multi-component photometric decomposition of 404 galaxies from the CALIFA Data Release 3. They represent all possible galaxies with no clear signs of i…

astro-ph.GA2016★ 272 cited

CALIFA, the Calar Alto Legacy Integral Field Area survey: IV. Third Public data release

S. F. Sánchez, R. García-Benito, S. Zibetti +60

This paper describes the Third Public Data Release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public,…

astro-ph.GA2015★ 98 cited

Automated Kinematic Modelling of Warped Galaxy Discs in Large Hi Surveys: 3D Tilted Ring Fitting of HI Emission Cubes

P. Kamphuis, G. I. G. Józsa, S-. H. Oh +5

Kinematical parameterisations of disc galaxies, employing emission line observations, are indispensable tools for studying the formation and evolution of galaxies. Future large-sca…

astro-ph.GA2015★ 2 cited

Structure, dynamical impact and origin of magnetic fields in nearby galaxies in the SKA era

Rainer Beck, Dominik Bomans, Sergio Colafrancesco +14

Magnetic fields are an important ingredient of the interstellar medium (ISM). Besides their importance for star formation, they govern the transport of cosmic rays, relevant to the…