11 citations · 19 across the 6 of their papers we have counts for
6 papers
Galaxy evolution through infrared and submillimeter spectroscopy: Measuring star formation and black hole accretion with JWST and ALMA
Sabrina Mordini, Luigi Spinoglio, Juan Antonio Fernández-Ontiveros
Rest-frame mid- to far-infrared spectroscopy is a powerful tool to study how galaxies formed and evolved, because a major part of their evolution occurs in heavily dust enshrouded…
Calibration of mid- to far-infrared spectral lines in galaxies
Sabrina Mordini, Luigi Spinoglio, Juan Antonio Fernández-Ontiveros
Mid- to far-infrared (IR) lines are suited to study dust obscured regions in galaxies, because IR spectroscopy allows us to explore the most hidden regions where heavily obscured s…
Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the Cosmic Noon with a SPICA-like mission
Luigi Spinoglio, Sabrina Mordini, Juan Antonio Fernandez-Ontiveros +31
We use the SPace Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to demonstrate how deep spectrophotometric surveys covering large cosmological volu…
The physics of Galaxy Evolution with SPICA observations
Luigi Spinoglio, Juan A. Fernandez-Ontiveros, Sabrina Mordini
The evolution of galaxies at Cosmic Noon (redshift 1<z<3) passed through a dust-obscured phase, during which most stars formed and black holes in galactic nuclei started to shine,…
Unveiling the physical processes that regulate Galaxy Evolution with SPICA observations
Luigi Spinoglio, Juan A. Fernández-Ontiveros, Sabrina Mordini
To study the dust obscured phase of the galaxy evolution during the peak of the Star Formation Rate (SFR) and the Black Hole Accretion Rate (BHAR) density functions (),…
Models of emission line profiles and spectral energy distributions to characterize the multi-frequency properties of active galactic nuclei
Giovanni La Mura, Marco Berton, Sina Chen +7
The spectra of Active Galactic Nuclei (AGNs) are often characterized by a wealth of emission lines with different profiles and intensity ratios that led to a complicated classifica…