activity
20172026
most citedThe Galactic Faraday depth sky revisited

56 citations · 220 across the 19 of their papers we have counts for

collaborators

21 papers

astro-ph.GA2026

The star formation history of Orion is structured and episodic

Alena Rottensteiner, João Alves, Stefan Meingast +6

The propagation of star formation throughout a molecular cloud complex can tell us much about its physical drivers and the importance of environmental versus intrinsic processes. W…

astro-ph.IM2026

Application of Bayesian Statistical Tools to SKA Telescopes Polarization Surveys to Study Magnetization of the Large-scale Structure of the Universe

Valentina Vacca, Sebastian Hutschenreuter, Andrea Cabriolu +18

Understanding cosmological magnetic fields requires a detailed knowledge of magnetism in the different environments of the large-scale structure of the Universe. Magnetic fields ar…

astro-ph.GA2026

Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies

Yik Ki Ma, Amit Seta, Aritra Basu +13

Magnetic fields in galaxies span decades in physical scale, from the coherent magnetic fields on galactic scales (> kpc) to the random magnetic fields from 100 pc to the resistive…

astro-ph.HE2026

EMU discovery of Thunder: a bow-shock PWN powered by PSR J1631-4722 escaping Nimbus SNR (G336.7+0.5)

S. Lazarević, C. Maitra, A. Ahmad +21

We report the discovery of a bow-shock pulsar wind nebula (PWN), dubbed Thunder, powered by the radio pulsar PSR J1631-4722 and projected within the Galactic supernova remnant (SNR…

astro-ph.IM2026

DEFROST: Detecting Excess in Faraday Rotation thrOugh Sophisticated analysis Techniques

Valentina Vacca, Sebastian Hutschenreuter, Andrea Cabriolu +7

Understanding origin and evolution of cosmological magnetic fields requires knowledge of magnetic fields in different extragalactic environments. In this context, a powerful tool i…

astro-ph.GA2026

The radial component of the local Galactic magnetic field in 3D

Lewis McCallum, Philipp Frank, Sebastian Hutschenreuter +9

We present a distance-resolved reconstruction of the local line-of-sight Galactic magnetic field, , by combining a 3D electron density () map derived from dust map-i…

astro-ph.GA2025★ 1 cited

The Polarisation Sky Survey of the Universe's Magnetism (POSSUM): Science Goals and Survey Description

B. M. Gaensler, G. H. Heald, N. M. McClure-Griffiths +57

The Australian SKA Pathfinder (ASKAP) offers powerful new capabilities for studying the polarised and magnetised Universe at radio wavelengths. In this paper, we introduce the Pola…

astro-ph.GA2025★ 2 cited

Modeling Local Bubble analogs II: Synthetic Faraday rotation maps

Efrem Maconi, Stefan Reissl, Juan D. Soler +4

Faraday rotation describes the change of the linear polarization angle of radiation passing through a magnetized plasma and it is quantified by the rotation measure (RM), which is…

astro-ph.GA2025

Improved constraints on the Faraday rotation towards eight fast radio bursts using dense grids of polarized radio galaxies

Ayush Pandhi, Bryan M. Gaensler, Ziggy Pleunis +6

We present 2-4 GHz observations of polarized radio galaxies towards eight fast radio bursts (FRBs), producing grids of Faraday rotation measure (RM) sources with sky densities of 9…

astro-ph.IM2024★ 2 cited

Interpolation techniques for reconstructing Galactic Faraday rotation

Affan Khadir, Ayush Pandhi, Sebastian Hutschenreuter +4

The line-of-sight structure of the Galactic magnetic field (GMF) can be studied using Faraday rotation measure (RM) grids. We analyze how the choice of interpolation kernel can aff…

astro-ph.IM2023★ 31 cited

RMTable2023 and PolSpectra2023: standards for reporting polarization and Faraday rotation measurements of radio sources

C. L. Van Eck, B. M. Gaensler, S. Hutschenreuter +11

Faraday rotation measures (RMs) have been used for many studies of cosmic magnetism, and in most cases having more RMs is beneficial for those studies. This has lead to development…

astro-ph.GA2023★ 21 cited

Disentangling the Faraday rotation sky

Sebastian Hutschenreuter, Marijke Haverkorn, Philipp Frank +2

Magnetic fields permeate the diffuse interstellar medium (ISM) of the Milky Way, and are essential to explain the dynamical evolution and current shape of the Galaxy. Magnetic fiel…

astro-ph.GA2023★ 45 cited

Detection of magnetic fields in the circumgalactic medium of nearby galaxies using Faraday rotation

V. Heesen, S. P. O'Sullivan, M. Brüggen +15

Context. The existence of magnetic fields in the circumgalactic medium (CGM) is largely unconstrained. Their detection is important as magnetic fields can have a significant impact…

astro-ph.GA2022★ 10 cited

A method for reconstructing the Galactic magnetic field using dispersion of fast radio bursts and Faraday rotation of radio galaxies

Ayush Pandhi, Sebastian Hutschenreuter, Jennifer West +2

With the rapid increase of fast radio burst (FRB) detections within the past few years, there is now a catalogue being developed for all-sky extragalactic dispersion measure (DM) o…

physics.ao-ph2021

Studying Bioluminescence Flashes with the ANTARES Deep Sea Neutrino Telescope

N. Reeb, S. Hutschenreuter, P. Zehetner +141

We develop a novel technique to exploit the extensive data sets provided by underwater neutrino telescopes to gain information on bioluminescence in the deep sea. The passive natur…

astro-ph.GA2021★ 4 cited

The Galactic Faraday rotation sky 2020

Sebastian Hutschenreuter, Craig S. Anderson, Sarah Betti +34

This work gives an update to existing reconstructions of the Galactic Faraday rotation sky by processing almost all Faraday rotation data sets available at the end of the year 2020…

astro-ph.GA2019★ 56 cited

The Galactic Faraday depth sky revisited

Sebastian Hutschenreuter, Torsten A. Enßlin

The Galactic Faraday depth sky is a tracer for both the Galactic magnetic field and the thermal electron distribution. It has been previously reconstructed from polarimetric measur…

astro-ph.HE2018★ 3 cited

Determining the composition of radio plasma via circular polarization: the prospects of the Cygnus A hot spots

Torsten A. Enßlin, Sebastian Hutschenreuter, Gopal-Krishna

The composition of the relativistic plasma produced in active galactic nuclei and ejected via powerful jets into the interstellar/intergalactic medium is still a major unsettled is…

astro-ph.CO2018★ 26 cited

The primordial magnetic field in our cosmic backyard

Sebastian Hutschenreuter, Sebastian Dorn, Jens Jasche +4

We reconstruct the 3D structure of magnetic fields, which were seeded by density perturbations during the radiation dominated epoch of the Universe and later on were evolved by str…

astro-ph.IM2017★ 2 cited

NIFTy 3 - Numerical Information Field Theory - A Python framework for multicomponent signal inference on HPC clusters

Theo Steininger, Jait Dixit, Philipp Frank +10

NIFTy, "Numerical Information Field Theory", is a software framework designed to ease the development and implementation of field inference algorithms. Field equations are formulat…

astro-ph.HE2017★ 14 cited

The Galaxy in circular polarization: all-sky radio prediction, detection strategy, and the charge of the leptonic cosmic rays

Torsten A. Enßlin, Sebastian Hutschenreuter, Valentina Vacca +1

The diffuse Galactic synchrotron emission should exhibit a low level of diffuse circular polarization (CP) due to the circular motions of the emitting relativistic electrons. This…