papers

Publications (24)

astro-ph.HE2025

A Square Kilometre Array Pulsar Census

E. F. Keane, V. Graber, L. Levin +8

Most of the pulsar science case with the Square Kilometre Array (SKA) depends on long-term precision pulsar timing of a large number of pulsars, as well as astrometric measurements…

astro-ph.GA2021

Apertif view of the OH Megamaser IRAS 10597+5926: OH 18 cm satellite lines in wide-area HI surveys

Kelley M. Hess, H. Roberts, H. Dénes +26

We present the serendipitous detection of the two main OH maser lines at 1667 and 1665 MHz associated with IRAS 10597+5926 at z = 0.19612 in the untargeted Apertif Wide-area Extrag…

astro-ph.HE2025

Understanding pulsar magnetospheres with the SKAO

L. S. Oswald, A. Basu, M. Chakraborty +22

The SKA telescopes will bring unparalleled sensitivity across a broad radio band, a wide field of view across the Southern sky, and the capacity for sub-arraying, all of which make…

astro-ph.GA2020

The best of both worlds: Combining LOFAR and Apertif to derive resolved radio spectral index images

R. Morganti, T. A. Oosterloo, M. Brienza +36

Supermassive black holes at the centres of galaxies can cycle through periods of activity and quiescence. Characterising the duty cycle of active galactic nuclei is crucial for und…

astro-ph.GA2025

The low-frequency flattening of the radio spectrum of giant HII regions in M 101

L. Gajović, V. Heesen, M. Brüggen +10

In galaxies, the flattening of the spectrum at low radio frequencies below 300 MHz has been the subject of some debate. A turnover at low frequencies could be caused by multiple ph…

astro-ph.GA2023

LOFAR discovery and wide-band characterisation of an ultra-steep spectrum AGN radio remnant associated with Abell 1318

A. Shulevski, M. Brienza, F. Massaro +15

We present the discovery of a very extended (550 kpc) and low-surface-brightness ( at 144 MHz) radio emission region in Abell 1318. These proper…

astro-ph.IM2021

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.IM2023

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.HE2021

A search for radio emission from double-neutron star merger GW190425 using Apertif

Olivér Boersma, Joeri van Leeuwen, Elizabeth A. K. Adams +26

Detection of the electromagnetic emission from coalescing binary neutron stars (BNS) is important for understanding the merger and afterglow. We present a search for a radio counte…

astro-ph.IM2023

An interference detection strategy for Apertif based on AOFlagger 3

A. R. Offringa, B. Adebahr, A. Kutkin +15

Context. Apertif is a multi-beam receiver system for the Westerbork Synthesis Radio Telescope that operates at 1.1-1.5 GHz, which overlaps with various radio services, resulting in…

astro-ph.HE2026

A Square Kilometre Array Pulsar Census

E. F. Keane, V. Graber, L. Levin +7

Most of the pulsar science case with the Square Kilometre Array (SKA) depends on long-term precision timing of a large number of pulsars, as well as their astrometric measurements…

astro-ph.GA2020

Extreme intra-hour variability of the radio source J1402+5347 discovered with Apertif

T. A. Oosterloo, H. K. Vedantham, A. M. Kutkin +27

The propagation of radio waves from distant compact radio sources through turbulent interstellar plasma in our Galaxy causes these sources to twinkle, a phenomenon called interstel…

astro-ph.IM2023

Survey-scale discovery-based research processes: Evaluating a bespoke visualisation environment for astronomical survey data

C. J. Fluke, D. Vohl, V. A. Kilborn +1

Next generation astronomical surveys naturally pose challenges for human-centred visualisation and analysis workflows that currently rely on the use of standard desktop display env…

astro-ph.IM2022

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.IM2022

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.HE2021

Dual-frequency single-pulse study of PSR B0950+08

A. V. Bilous, J. M. Griessmeier, T. Pennucci +33

PSR B0950+08 is a bright non-recycled pulsar whose single-pulse fluence variability is reportedly large. Based on observations at two widely separated frequencies, 55 MHz (NenuFAR)…

astro-ph.IM2021

Apercal -- The Apertif Calibration Pipeline

B. Adebahr, R. Schulz, T. J. Dijkema +33

Apertif (APERture Tile In Focus) is one of the Square Kilometre Array (SKA) pathfinder facilities. The Apertif project is an upgrade to the 50-year-old Westerbork Synthesis Radio T…

astro-ph.HE2023

Searching for FRB persistent radio source counterparts in dwarf galaxies using LOFAR

D. Vohl, H . K. Vedantham, J. W. T. Hessels +1

The repeating FRB 20121102A was localized to a star-forming region in a dwarf galaxy and found to be co-located with a persistent radio source (PRS). FRB 20190520B is only the seco…

astro-ph.HE2026

Understanding Pulsar Magnetospheres with the SKAO

L. S. Oswald, A. Basu, M. Chakraborty +21

The SKA telescopes will bring unparalleled sensitivity across a broad radio band, a wide field of view across the Southern sky, and the capacity for sub-arraying, all of which make…

astro-ph.HE2024

Topology of Pulsar Profiles (ToPP). I. Graph theory method and classification of the EPN

D. Vohl, J. van Leeuwen, Y. Maan

Some of the most important information on a radio pulsar is derived from its average pulse profile. Many early pulsar studies were necessarily based on only few such profiles. Ther…

astro-ph.HE2020

Repeating fast radio bursts with WSRT/Apertif

L. C. Oostrum, Y. Maan, J. van Leeuwen +40

Repeating fast radio bursts (FRBs) present excellent opportunities to identify FRB progenitors and host environments, as well as decipher the underlying emission mechanism. Detaile…

astro-ph.GA2022

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.IM2022

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.HE2023

A LOFAR sample of luminous compact sources coincident with nearby dwarf galaxies

D. Vohl, H. K. Vedantham, J. W. T. Hessels +5

The vast majority of extragalactic compact continuum radio sources are associated with star formation or jets from (super)massive black holes and, as such, are more likely to be fo…