activity
20022026
most citedThe LOFAR Two-metre Sky Survey -- V. Second data release

489 citations · 7.2k across the 173 of their papers we have counts for

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Showing 2024Show all

18 papers · 1 filter

astro-ph.GA2024

On the kinematic and thermodynamic state of clouds in complex wind-multi-cloud environments using a Friends-of-Friends analysis

Andrei Antipov, Wladimir E. Banda-Barragán, Yuval Birnboim +3

We investigate the interaction between a shock-driven hot wind and a cold multi-cloud layer, for conditions commonly found in interstellar and circumgalactic gas. We present a meth…

astro-ph.GA2024★ 19 cited

The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies

Yi Zhang, Johan Comparat, Gabriele Ponti +17

The circumgalactic medium (CGM), as the gas repository for star formation, might contain the answer to the mysterious galaxy quenching and bimodal galaxy population origin. We meas…

astro-ph.GA2024

A spatially-resolved spectral analysis of giant radio galaxies with MeerKAT

K. K. L. Charlton, J. Delhaize, K. Thorat +13

In this study we report spatially resolved, wideband spectral properties of three giant radio galaxies (GRGs) in the COSMOS field: MGTC J095959.63+024608.6 , MGTC J100016.84+015133…

astro-ph.IM2024★ 3 cited

Simulating images of radio galaxies with diffusion models

Tobias Vičánek Martínez, Nicolás Barón Pérez, Marcus Brüggen

With increasing amounts of data in astronomy, automated analysis methods have become crucial. Synthetic data are required for developing and testing such methods. Current simulatio…

astro-ph.GA2024★ 7 cited

CHANG-ES XXXIV: a 20 kpc radio bubble in the halo of the star-forming galaxy NGC 4217

V. Heesen, T. Wiegert, J. Irwin +11

Cosmic rays may be dynamically very important in driving large-scale galactic winds. Edge-on galaxies give us an outsider's view of the radio halo, which shows the presence of extr…

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…