activity
20242026
collaborators

6 papers

gr-qc2026

How much dark matter really matters?

Jenny Wagner

Strong gravitational lensing is a key probe to trace dark matter. It assumes that mass curves spacetime so that light from a background source is deflected on its way to the observ…

astro-ph.GA2026

Hamilton's Object Revisited: A challenging source redshift of a strong lensing configuration

Jenny Wagner, Emilio E. Falco

Low-resolution spectrographs used to have difficulties in determining redshifts of galaxies at and . Spectral emission and absorption lines of magnesium and…

astro-ph.CO2025

The Binary Ballet: Mapping Local Expansion Around M81 & M82

Jenny Wagner, David Benisty, Igor D. Karachentsev

This study of the M81 complex and its Hubble flow delivers new and improved Tip of the Red Giant Branch (TRGB)-based distances for nine member galaxies, yielding a total of 58 gala…

astro-ph.CO2025

Unveiling the Coma Cluster Structure: From the Core to the Hubble Flow

David Benisty, Jenny Wagner, Sandeep Haridasu +1

The Coma cluster, embedded in a cosmic filament, is a complex and dynamically active structure in the local Universe. Applying a density-based member selection dbscan to data from…

astro-ph.GA2025

Galaxy infall models for arbitrary velocity directions

Jenny Wagner, David Benisty

For most galaxies in the cosmos, our knowledge of their motion is limited to line-of-sight velocities from redshift observations. To determine the radial velocity between two galax…

gr-qc2024

Observables of super-extremal black holes: challenging Cosmic Censorship to comprehend the Cosmological Constant

Jenny Wagner

Einstein's Field Equations have proven applicable across many scales, from black holes to cosmology. Even the mysterious Cosmological Constant found a physical interpretation in th…