activity
20182020
most citedLow-frequency Faraday rotation measures towards pulsars using LOFAR: probing the 3-D Galactic halo magnetic field

108 citations · 167 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.GA202017 cited

Discovery of a Thirty-Degree Long Ultraviolet Arc in Ursa Major

A. Bracco, R. A. Benjamin, M. I. R. Alves +6

Our view of the interstellar medium of the Milky Way and the universe beyond is affected by the structure of the local environment in the Solar neighborhood. Here, we present the d…

astro-ph.GA201942 cited

Diffuse polarized emission in the LOFAR Two-meter Sky Survey

C. L. Van Eck, M. Haverkorn, M. I. R. Alves +13

Faraday tomography allows us to map diffuse polarized synchrotron emission from our Galaxy and use it to interpret the magnetic field in the interstellar medium (ISM). We have appl…

astro-ph.GA2019108 cited

Low-frequency Faraday rotation measures towards pulsars using LOFAR: probing the 3-D Galactic halo magnetic field

C. Sobey, A. V. Bilous, J-M. Grießmeier +22

We determined Faraday rotation measures (RMs) towards 137 pulsars in the northern sky, using Low-Frequency Array (LOFAR) observations at 110-190 MHz. This low-frequency RM catalogu…

astro-ph.GA2018

Low frequency measurements of synchrotron absorbing HII regions and modeling of observed synchrotron emissivity

I. M. Polderman, M. Haverkorn, T. R. Jaffe +1

Cosmic rays (CRs) and magnetic fields are dynamically important components in the Galaxy, and their energy densities are comparable to that of the turbulent interstellar gas. The i…

astro-ph.GA2018

The Local Bubble: a magnetic veil to our Galaxy

M. I. R. Alves, F. Boulanger, K. Ferriere +1

The magnetic field in the local interstellar medium does not follow the large-scale Galactic magnetic field. The local magnetic field has probably been distorted by the Local Bubbl…