activity
19962026
most citedThe Star Formation Efficiency in Nearby Galaxies: Measuring Where Gas Forms Stars Effectively

1.9k citations · 10.7k across the 45 of their papers we have counts for

collaborators

45 papers

astro-ph.GA2026

HI rotation curves and mass-size relation for 568 galaxies from the Apertif Wide-area Extragalactic Survey

Konstantin Haubner, Federico Lelli, Enrico Di Teodoro +13

The extended HI rotation curves of galaxies are one of the most powerful tools for studying galaxy evolution and for testing different dark matter and modified gravity models. Howe…

astro-ph.IM2026

Options for Compression of radio interferometry data: lossy compression of visibilities and lossless compression of uv-visibility grids for the MHONGOOSE survey

Richard Dodson, Jonghwan Rhee, W. J. G. de Blok +6

Next generation radio astronomy telescopes are challenging existing data reduction paradigms. With ever more antennas, larger bandwidths, and sometimes multiple primary beams, they…

astro-ph.GA2026

Deep HI observations of cold gas inflow and outflow

W. J. G. de Blok, D. B. Fisher, K. Tachihara +8

A major question in galaxy evolution is how galaxies acquire sufficient gas to sustain their star formation rates. HI observations with high angular resolution and sensitivity to v…

astro-ph.GA2026

FEASTS and MHONGOOSE: HI Column Density Distribution at for

Jing Wang, Xuchen Lin, Ze-Zhong Liang +24

We present the first HI column density distribution function, , extending down to . This was derived from high-s…

astro-ph.HE2023

A new method for short duration transient detection in radio images: Searching for transient sources in MeerKAT data of NGC 5068

S. Fijma, A. Rowlinson, R. A. M. J. Wijers +12

Transient surveys are a vital tool in exploring the dynamic universe, with radio transients acting as beacons for explosive and highly energetic astrophysical phenomena. However, p…

astro-ph.IM2023★ 6 cited

Apertif 1.4 GHz continuum observations of the Boötes field and their combined view with LOFAR

A. M. Kutkin, T. A. Oosterloo, R. Morganti +17

We present a new image of a 26.5 square degree region in the Boötes constellation obtained at 1.4 GHz using the Aperture Tile in Focus (Apertif) system on the Westerbork Synthesis…

astro-ph.IM2022★ 14 cited

Continuum source catalog for the first APERTIF data release

A. M. Kutkin, T. A. Oosterloo, R. Morganti +25

The first data release of Apertif survey contains 3074 radio continuum images covering a thousand square degrees of the sky. The observations were performed during August 2019 to J…

astro-ph.IM2022★ 42 cited

First release of Apertif imaging survey data

Elizabeth A. K. Adams, B. Adebahr, W. J. G. de Blok +56

(Abridged) Apertif is a phased-array feed system for WSRT, providing forty instantaneous beams over 300 MHz of bandwidth. A dedicated survey program started on 1 July 2019, with th…

astro-ph.GA2022★ 8 cited

Seeing the forest and the trees: a radio investigation of the ULIRG Mrk 273

Pranav Kukreti, Raffaella Morganti, Marco Bondi +19

Galaxy mergers have been observed to trigger nuclear activity by feeding gas to the central supermassive black hole. One such class of objects are Ultra Luminous InfraRed Galaxies…

astro-ph.IM2022★ 6 cited

Characterising the Apertif primary beam response

H. Dénes, K. M. Hess, E. A. K. Adams +27

Context. Phased Array Feeds (PAFs) are multi element receivers in the focal plane of a telescope that make it possible to form simultaneously multiple beams on the sky by combining…

astro-ph.GA2022★ 12 cited

The Apertif science verification campaign - Characteristics of polarised radio sources

B. Adebahr, A. Berger, E. A. K. Adams +24

We analyse five early science datasets from the APERture Tile in Focus (Apertif) phased array feed system to verify the polarisation capabilities of Apertif in view of future large…

astro-ph.IM2021★ 1 cited

Apertif, Phased Array Feeds for the Westerbork Synthesis Radio Telescope

W. A. van Cappellen, T. A. Oosterloo, M. A. W. Verheijen +87

We describe the APERture Tile In Focus (Apertif) system, a phased array feed (PAF) upgrade of the Westerbork Synthesis Radio Telescope which has transformed this telescope into a h…

astro-ph.GA2017★ 96 cited

Physical Properties of Molecular Clouds at 2 parsec Resolution in the Low-Metallicity Dwarf Galaxy NGC 6822 and the Milky Way

Andreas Schruba, Adam K. Leroy, J. M. Diederik Kruijssen +6

We present the ALMA survey of CO(2-1) emission from the 1/5 solar metallicity, Local Group dwarf galaxy NGC 6822. We achieve high (0.9 arcsec ~ 2 pc) spatial resolution while cover…

astro-ph.GA2015★ 2 cited

Magnetic Field Tomography in Nearby Galaxies with the Square Kilometre Array

George Heald, Rainer Beck, W. J. G. de Blok +16

Magnetic fields play an important role in shaping the structure and evolution of the interstellar medium (ISM) of galaxies, but the details of this relationship remain unclear. Wit…

astro-ph.GA2014★ 41 cited

A low HI column density filament in NGC 2403: signature of interaction or accretion

W. J. G. de Blok, Katie M. Keating, D. J. Pisano +6

Observed HI accretion around nearby galaxies can only account for a fraction of the gas supply needed to sustain the currently observed star formation rates. It is possible that ad…

astro-ph.CO2013★ 117 cited

A high-dispersion molecular gas component in nearby galaxies

Anahi Caldu-Primo, Andreas Schruba, Fabian Walter +5

We present a comprehensive study of the velocity dispersion of the atomic (HI) and molecular (H2) gas components in the disks (R < R25) of a sample of 12 nearby spiral galaxies wit…

astro-ph.CO2012★ 23 cited

Disk Stability and Neutral Hydrogen as a Tracer of Dark Matter

Gerhardt R. Meurer, Zheng Zheng, W. J. G. de Blok

We derive the projected surface mass distribution Sigma_M for spherically symmetric mass distributions having an arbitrary rotation curve. For a galaxy with a flat rotation curve a…

astro-ph.CO2012★ 262 cited

Low CO Luminosities in Dwarf Galaxies

Andreas Schruba, Adam K. Leroy, Fabian Walter +10

[Abridged] We present maps of CO 2-1 emission covering the entire star-forming disks of 16 nearby dwarf galaxies observed by the IRAM HERACLES survey. The data have 13 arcsec angul…

astro-ph.CO2012★ 203 cited

Estimating the Star Formation Rate at 1 kpc Scales in Nearby Galaxies

Adam K. Leroy, Frank Bigiel, W. J. G. de Blok +9

Using combinations of Hα, ultraviolet (UV), and infrared (IR) emission, we estimate the star formation rate (SFR) surface density, Σ_SFR, at 1 kpc resolution for 30 disk galaxies t…

astro-ph.CO2012★ 34 cited

On the Origin of the Supergiant HI Shell and Putative Companion in NGC 6822

John M. Cannon, Erin M. O'Leary, Daniel R. Weisz +6

We present new Hubble Space Telescope Advanced Camera for Surveys imaging of six positions spanning 5.8 kpc of the HI major axis of the Local Group dIrr NGC 6822, including both th…

astro-ph.CO2011★ 91 cited

Improved Modeling of the Mass Distribution of Disk Galaxies by the Einasto Halo Model

Laurent Chemin, W. J. G. de Blok, Gary A. Mamon

(Abridged) The analysis of the rotation curves (RCs) of spiral galaxies provides an efficient diagnostic for studying the properties of dark matter halos and their relations with t…

astro-ph.CO2011★ 555 cited

A Molecular Star Formation Law in the Atomic Gas Dominated Regime in Nearby Galaxies

Andreas Schruba, Adam K. Leroy, Fabian Walter +11

We use the IRAM HERACLES survey to study CO emission from 33 nearby spiral galaxies down to very low intensities. Using atomic hydrogen (HI) data, mostly from THINGS, we predict th…

astro-ph.CO2011★ 41 cited

Quantified HI Morphology III: Merger Visibility Times from HI in Galaxy Simulations

B. W. Holwerda, N. Pirzkal, T. J. Cox +5

Major mergers of disk galaxies are thought to be a substantial driver in galaxy evolution. To trace the fraction and the rate galaxies are in mergers over cosmic times, several obs…

astro-ph.CO2011★ 13 cited

Quantified HI Morphology V: HI Disks in the Virgo Cluster

B. W. Holwerda, N. Pirzkal, W. J. G. de Blok +1

We explore the quantified morphology of atomic hydrogen (HI) disks in the Virgo cluster. These galaxies display a wealth of phenomena in their Hi morphology, e.g., tails, truncatio…