most citedA New Uncertainty Scheme for Galaxy Distances from Flow Models

4 citations · 4 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025

The baryonic mass-size relation of galaxies. I. A dichotomy in star-forming galaxy disks

Zichen Hua, Federico Lelli, Enrico Di Teodoro +2

The mass-size relations of galaxies are generally studied considering only stars or only gas separately. Here we study the baryonic mass-size relation of galaxies from the SPARC da…

astro-ph.CO2025

Mass models of galaxy clusters from a non-parametric weak-lensing reconstruction

Tobias Mistele, Federico Lelli, Stacy McGaugh +2

We study the CLASH sample of galaxy clusters using a new deprojection method for weak gravitational lensing observations. This method is non-parametric, allowing us to infer mass p…

astro-ph.CO20254 cited

A New Uncertainty Scheme for Galaxy Distances from Flow Models

Konstantin Haubner, Federico Lelli, Enrico Di Teodoro +3

The systemic velocity or redshift of galaxies is a convenient tool to calculate their distances in the absence of primary methods, but the uncertainties on these flow distances may…

astro-ph.GA2025

The Baryonic Tully-Fisher Relation II: Stellar Mass Models

Francis Duey, James Schombert, Stacy McGaugh +1

We present new color- (mass-to-light) models to convert WISE W1 fluxes into stellar masses. We outline a range of possible star formation histories and chemical evolution scen…

astro-ph.GA2024

BIG-SPARC: The new SPARC database

Konstantin Haubner, Federico Lelli, Enrico Di Teodoro +5

The Surface Photometry and Accurate Rotation Curves (SPARC) database has provided the community with mass models for 175 nearby galaxies, allowing different research teams to test…

astro-ph.GA2024

The empirical laws of galaxy dynamics: from gas kinematics to weak lensing

Federico Lelli, Tobias Mistele, Stacy S. McGaugh +2

Galaxies obey a set of strict dynamical laws, which imply a close coupling between the visible matter (stars and gas) and the observed dynamics (set by dark matter in the standard…