activity
20132026
most citedVelocity-resolved reverberation mapping of five bright Seyfert 1 galaxies

101 citations · 301 across the 49 of their papers we have counts for

collaborators

51 papers

astro-ph.IM2026

Towards First Light for MICADO: Validation of the PSF-R service with real data

Matteo Simioni, Luca Cortese, Roland Wagner +12

MICADO, one of the ELT first-light instruments, will rely on point-spread-function reconstruction (PSF-R) to meet scientific requirements, especially for SCAO observations of targe…

astro-ph.IM2026

The MICADO first light imager for the ELT: the PSF Reconstruction Software

Andrea Grazian, Fernando Pedichini, Matteo Simioni +14

The MICADO instrument for the ESO ELT will provide Adaptive Optics (AO) diffraction-limited NIR imaging and spectroscopy. A critical component of MICADO is the Point Spread Functio…

astro-ph.GA2026

The MICADO first light imager for the ELT: Simulated Observations of Star Forming Clumps at Cosmic Noon

Matteo Simioni, Carmelo Arcidiacono, Andrea Grazian +18

Galaxies at redshift z2-6 exhibit prominent star-forming regions (clumps). Characterisation of these galactic structures requires both high sensitivity and spatial resolution…

astro-ph.IM2026

Structural, thermal and optical tolerance analysis of SHARP, a near infrared spectrograph for next generation telescope

H. Mahmoodzadeh, P. Saracco, I. DI Antonio +15

The design and verification of cryogenic near-infrared spectrographs require rigorous multidisciplinary analyses to ensure optical performance under realistic operational condition…

astro-ph.IM2026

MORFEO: Advancing Towards Final Design

Lorenzo Busoni, Guido Agapito, Marco Bonaglia +106

The Multiconjugate adaptive Optics Relay For ELT Observations (MORFEO) is a first-generation adaptive optics module for the Extremely Large Telescope (ELT), designed to deliver a d…

astro-ph.GA2026

Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP

E. Bortolas, E. Portaluri, E. Dalla Bonta' +3

Massive black hole (MBH) binaries form as a result of galaxy mergers and can coalesce into a single MBH by emitting gravitational waves detectable by LISA and pulsar timing array c…