activity
19992025
most citedEuclid. I. Overview of the Euclid mission

550 citations · 1.9k across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.HE2025★ 3 cited

Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"

Joanna M. Rankin, Vyacheslav Zakharenko, Oleg Ulyanov +9

PSR B1237+25 is perhaps the canonical example of a pulsar with a core/double cone profile. Moreover, it is bright with little spectral turnover, and its profile perhaps uniquely re…

astro-ph.GA2024★ 6 cited

Monster radio jet (>66 kpc) observed in quasar at z5

Anniek J. Gloudemans, Frits Sweijen, Leah K. Morabito +6

We present the discovery of a large extended radio jet associated with the extremely radio-loud quasar J1601+3102 at from sub-arcsecond resolution imaging at 144 MHz with…

astro-ph.CO2024★ 550 cited

Euclid. I. Overview of the Euclid mission

Euclid Collaboration, Y. Mellier, Abdurro'uf +1134

The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Eucl…

astro-ph.IM2023★ 40 cited

The LOFAR LBA Sky Survey II. First data release

F. de Gasperin, H. W. Edler, W. L. Williams +27

The Low Frequency Array (LOFAR) is the only existing radio interferometer able to observe at ultra-low frequencies (<100 MHz) with high resolution (<15") and high sensitivity (<1 m…

astro-ph.GA2020★ 29 cited

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.HE2018★ 18 cited

Blazars in the LOFAR Two-Metre Sky Survey First Data Release

S. Mooney, J. Quinn, J. R. Callingham +13

Historically, the blazar population has been poorly understood at low frequencies because survey sensitivity and angular resolution limitations have made it difficult to identify m…