7 citations · 18 across the 7 of their papers we have counts for
8 papers
Recently launched AGN-driven outflow in a lensed quiescent galaxy at Cosmic Noon
Letizia Bugiani, Andrew B. Newman, Sirio Belli +11
We analyze JWST/NIRSpec IFU spectroscopy of MRG-M0150, a gravitationally lensed, massive quiescent galaxy at from the INQUEST-JWST survey. Thanks to the combination of lens…
Signatures and bias assessment of rotation in galaxy cluster members
Davide Castellani, Giovanni Ferrami, Claudio Grillo +1
We investigate the possible presence of systematic rotation in the member galaxies of a sample of 17 nearby (), rich (at least 80 identified members) Abell clusters. We also…
Galaxy cluster virial quantities from extrapolating strong lensing mass profiles
Enrico Maraboli, Claudio Grillo, Pietro Bergamini +1
We study the radial total mass profiles of nine massive galaxy clusters ( M) in the redshift range . These clusters were obse…
The GLASS-JWST Early Release Science Programme: The NIRISS Spectroscopic Catalogue
Peter J. Watson, Benedetta Vulcani, Tommaso Treu +18
We present a spectroscopic redshift catalogue of sources in the Abell 2744 cluster field, derived from JWST/NIRISS observations taken as part of the GLASS-JWST Early Release Scienc…
A stellar dynamical mass measurement of an inactive black hole at redshift 2
Andrew B. Newman, Meng Gu, Sirio Belli +34
Supermassive black holes and their host galaxies grow together over time, producing correlations between the black hole mass and various galaxy properties. Determining the evolutio…
Accelerating lensed quasar discovery and modeling with physics-informed variational autoencoders
Irham T. Andika, Stefan Schuldt, Sherry H. Suyu +5
Strongly lensed quasars provide valuable insights into the rate of cosmic expansion, the distribution of dark matter in foreground deflectors, and the characteristics of quasar hos…
Spherical bias on the 3D reconstruction of the ICM density profile in galaxy clusters
I. Veronesi, I. Bartalucci, E. Rasia +9
X-ray observations of galaxy clusters are routinely used to derive radial distributions of ICM thermdynamical properties such as density and temperature. However, observations allo…
Does the Fe L-shell blend bias abundance measurements in intermediate-temperature clusters?
G. Riva, S. Ghizzardi, S. Molendi +5
In intermediate-temperature (T = 2.5 - 4.5 keV) galaxy clusters, abundance measurements are almost-equally driven by Fe K and L transitions, at 6.7 keV and 0.9 - 1.3 keV, re…