Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Astronomy, and Cluster (spacecraft).
A pristine, star-forming complex at <i>z</i> = 4.19
<i>Euclid</i> preparation
Cosmic chronometers with galaxy clusters: A new avenue for multi-probe cosmology
Euclid preparation. Impact of redshift distribution uncertainties on the joint analysis of photometric galaxy clustering and weak gravitational lensing
Euclid preparation. Non-Gaussianity of 2-pt statistics likelihood: Parameter inference with a non-Gaussian likelihood in Fourier and configuration space
Euclid Quick Data Release (Q1). AgileLens: A scalable CNN-based pipeline for strong gravitational lens identification
<i>Euclid</i>: Early Release Observations – Programme overview and pipeline for compact- and diffuse-emission photometry
<i>Euclid</i> preparation
JWST spectroscopic confirmation of the Cosmic Gems arc at <i>z</i> = 9.625
<i>Euclid</i> preparation
Parametric strong lensing model of the galaxy cluster Abell 2390 from <i>Euclid</i> and MUSE observations
<i>Euclid</i>: The search for primordial features
<i>Euclid</i> preparation
<i>Euclid</i>: Constraining linearly scale-independent modifications of gravity with the spectroscopic and photometric primary probes
<i>Euclid</i> preparation
<i>Euclid</i> preparation
<i>Euclid</i> preparation
<i>Euclid</i> preparation
<i>Euclid</i> preparation
Augmenting the power of time-delay cosmography in lens galaxy clusters by probing their member galaxies
<i>Euclid</i> preparation
Euclid preparation. Sensitivity to neutrino parameters
<i>Euclid</i> preparation
<i>Euclid</i> preparation
Euclid: Field-level inference of primordial non-Gaussianity and cosmic initial conditions
<i>Euclid</i> preparation
Euclid preparation XLVI. The Near-IR Background Dipole Experiment with Euclid
Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys
Euclid preparation: Determining the weak lensing mass accuracy and precision for galaxy clusters
Early Results from GLASS-JWST. XIX. A High Density of Bright Galaxies at z ≈ 10 in the A2744 Region