Constraining clumpy dusty torus models using optimized filter sets
Recent success in explaining several properties of the dusty torus around the central engine of active galactic nuclei has been gathered with the assumption of...
Constraining cosmic rays and magnetic fields in the Perseus galaxy cluster with TeV observations by the MAGIC telescopes
Galaxy clusters are being assembled today in the most energetic phase of hierarchical structure formation which manifests itself in powerful shocks that...
Constraining Galaxy Evolution with Scaling Relations
An ongoing study is presented in which a photometric non-linear Scaling Relation of Early-Type Galaxies (ETGs) is proposed to carry out a consistency test on...
Constraining nuclear star cluster formation using MUSE-AO observations of the early-type galaxy FCC 47
Context. Nuclear star clusters (NSCs) are found in at least 70% of all galaxies, but their formation path is still unclear. In the most common scenarios, NSCs...
Constraining stellar population parameters from narrow band photometric surveys using convolutional neural networks
Upcoming large-area narrow band photometric surveys, such as Javalambre Physics of the Accelerating Universe Astrophysical Survey (J-PAS), will enable us to...
Constraining the Epoch of Reionization from the Observed Properties of the High-z Universe
We combine observational data on a dozen independent cosmic properties at high-z with the information on reionization drawn from the spectra of distant luminous...
Constraining the formation of inner bars: photometry, kinematics and stellar populations in NGC 357
Double-barred galaxies are common in the local Universe, with approximately one-third of barred spirals hosting a smaller, inner bar. Nested bars have been...
Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias
We present a method to produce mock galaxy catalogues with efficient perturbation theory schemes, which match the number density, power spectra and bispectra in...