activity
20122023
most citedThe dust-continuum size of TNG50 galaxies at : a comparison with the distribution of stellar light, stars, dust and H

74 citations · 240 across the 10 of their papers we have counts for

collaborators

10 papers

quant-ph2023★ 14 cited

Guided quantum walk

Sebastian Schulz, Dennis Willsch, Kristel Michielsen

We utilize the theory of local amplitude transfers (LAT) to gain insights into quantum walks (QWs) and quantum annealing (QA) beyond the adiabatic theorem. By representing the eige…

astro-ph.CO2023★ 19 cited

A case study for measuring the relativistic dipole of a galaxy cross-correlation with the Dark Energy Spectroscopic Instrument

Camille Bonvin, Francesca Lepori, Sebastian Schulz +3

The data on spectroscopic galaxy clustering collected by the Dark Energy Spectroscopic Instrument (DESI) will allow the significant detection of subtle features in the galaxy two-p…

astro-ph.CO2023★ 2 cited

Glass-Like Random Catalogues for Two-Point Estimates on the Light Cone

Sebastian Schulz

We introduce grlic, a publicly available Python tool for generating glass-like point distributions with a radial density profile as it is observed in large-scale surveys of…

astro-ph.HE2022★ 11 cited

Diffusion of cosmic-ray electrons in M 51 observed with LOFAR at 54 MHz

V. Heesen, F. de Gasperin, S. Schulz +8

Context. The details of cosmic-ray transport have a strong impact on galaxy evolution. The peak of the cosmic-ray energy distribution is observable in the radio continuum using the…

astro-ph.CO2022★ 26 cited

Euclid: Modelling massive neutrinos in cosmology -- a code comparison

J. Adamek, R. E. Angulo, C. Arnold +133

The measurement of the absolute neutrino mass scale from cosmological large-scale clustering data is one of the key science goals of the Euclid mission. Such a measurement relies o…

astro-ph.GA2022★ 22 cited

Nearby galaxies in the LOFAR Two-metre Sky Survey II. The magnetic field-gas relation

V. Heesen, T. -L. Klocke, M. Brüggen +8

Context. Magnetic fields are key to understand galaxy evolution, regulating stellar feedback and star formation in galaxies. Aims. We probe the origin of magnetic fields in late-ty…

math.DG2022★ 1 cited

Nilpotent Higgs bundles and families of flat connections

Sebastian Schulz

We investigate -families of flat connections whose leading term is a nilpotent Higgs field. Examples of such families include real twistor lines and families ari…

astro-ph.GA2021★ 74 cited

The dust-continuum size of TNG50 galaxies at : a comparison with the distribution of stellar light, stars, dust and H

Gergö Popping, Annalisa Pillepich, Gabriela Calistro Rivera +6

We present predictions for the extent of the dust-continuum emission of thousands of main-sequence galaxies drawn from the TNG50 simulation between . To this aim, we couple…

astro-ph.GA2020★ 37 cited

A redshift-dependent IRX- dust attenuation relation for TNG50 galaxies

Sebastian Schulz, Gergö Popping, Annalisa Pillepich +4

We study the relation between the UV-slope, , and the ratio between the infrared- and UV-luminosities (IRX) of galaxies from TNG50, the latest installment of the IllustrisTNG ga…

hep-th2012★ 34 cited

On the Unlikeliness of Multi-Field Inflation: Bounded Random Potentials and our Vacuum

Diana Battefeld, Thorsten Battefeld, Sebastian Schulz

Based on random matrix theory, we compute the likelihood of saddles and minima in a class of random potentials that are softly bounded from above and below, as required for the val…