activity
20222026
most citedAccuracy and precision of triaxial orbit models I: SMBH mass, stellar mass and dark-matter halo

15 citations · 49 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Triaxial Schwarzschild Models of Brightest Cluster Galaxies with Long-Slit LBT Data

Stefano de Nicola, Roberto P. Saglia, Jens Thomas +3

We present new long-slit stellar kinematics for a sample of 21 Brightest Cluster Galaxies (BCGs) and triaxial Schwarzschild models for 16 of these objects using our orbit modelling…

astro-ph.GA2023★ 13 cited

The isotropic center of NGC 5419 -- A core in formation?

Bianca Neureiter, Jens Thomas, Antti Rantala +5

With its cored surface brightness profile, the elliptical galaxy NGC 5419 appears as a typical high-mass early-type galaxy (ETG). However, the galaxy hosts two distinct nuclei in i…

astro-ph.GA2022★ 15 cited

Accuracy and precision of triaxial orbit models I: SMBH mass, stellar mass and dark-matter halo

B. Neureiter, S. de Nicola, J. Thomas +3

We investigate the accuracy and precision of triaxial dynamical orbit models by fitting two dimensional mock observations of a realistic N-body merger simulation resembling a massi…

astro-ph.CO2022★ 12 cited

Euclid preparation: XX. The Complete Calibration of the Color-Redshift Relation survey: LBT observations and data release

Euclid Collaboration, R. Saglia, S. De Nicola +183

The Complete Calibration of the Color-Redshift Relation survey (C3R2) is a spectroscopic programme designed to empirically calibrate the galaxy color-redshift relation to the Eucli…

astro-ph.GA2022★ 9 cited

Intrinsic shapes of Brightest Cluster Galaxies

Stefano de Nicola, Roberto P. Saglia, Jens Thomas +5

We discuss the statistical distribution of galaxy shapes and viewing angles under the assumption of triaxiality by deprojecting observed Surface Brightness (SB) profiles of 56 Brig…