activity
19992025
most citedNew constraints on a triaxial model of the Galaxy

85 citations · 89 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2025

Towards measuring astrophysical third order correlation functions with the H.E.S.S. optical intensity interferometer

Andreas Zmija, Gisela Anton, Christopher Ingenhuett +7

The closure phase, the sum of the three Fourier phases in a telescope triangle, is an important tool in astronomical interferometry, helping to reconstruct the geometries of the ob…

astro-ph.IM2025

Probing Stellar Kinematics with the Time-Asymmetric Hanbury Brown and Twiss Effect

Lucijana Stanic, Ivan Cardea, Edoardo Charbon +11

Intensity interferometry (II) offers a powerful means to observe stellar objects with a high resolution. In this work, we demonstrate that II can also probe internal stellar kinema…

astro-ph.GA2025★ 1 cited

Dark Matter Particle Flux in a Dynamically Self-consistent Milky Way Model

Lucijana Stanic, Mark Eberlein, Stanislav Linchakovskyy +5

We extend a recently developed dynamically self-consistent model of the Milky Way constrained by observations from the Gaia observatory to include a radially anisotropic component…

astro-ph.GA2024

Reconciling concentration to virial mass relations

Dominik Leier, Ignacio Ferreras, Andrea Negri +1

The concentration-virial mass (c-M) relation is a fundamental scaling relation within the standard cold dark matter (CDM) framework well established in numerical simulations. Ho…

astro-ph.HE2024★ 3 cited

Bridging the micro-Hz gravitational wave gap via Doppler tracking with the Uranus Orbiter and Probe Mission: Massive black hole binaries, early universe signals and ultra-light dark matter

Lorenz Zwick, Deniz Soyuer, Daniel J. D'Orazio +6

With the recent announcement by NASA's \textit{Planetary Science and Astrobiology Decadal Survey 2023-2032}, a priority flagship mission to the planet Uranus is anticipated. Here,…

astro-ph1999★ 85 cited

New constraints on a triaxial model of the Galaxy

M. Sevenster, P. Saha, D. Valls-Gabaud +1

We determine the values of parameters of an N-body model for the Galaxy developed by Fux via comparison with an unbiased, homogeneous sample of OH/IR stars. Via Monte-Carlo simulat…