Sabrina Mordini
INAF
9 Papers
1 Citations
Sabrina Mordini is an academic researcher from INAF. The author has contributed to research in topics: Star formation & Galaxy. The author has an hindex of 1, co-authored 8 publications. Previous affiliations of Sabrina Mordini include Sapienza University of Rome.
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Papers
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,J. A. Fernández-Ontiveros,Almudena Alonso-Herrero,Lee Armus,L. Bisigello,Francesco Calura,Francisco J. Carrera,Asantha Cooray,Helmut Dannerbauer,Roberto Decarli,Eiichi Egami,David Elbaz,Alberto Franceschini,Eduardo Gonzalez Alfonso,L. Graziani,Carlotta Gruppioni,Evanthia Hatziminaoglou,Hidehiro Kaneda,Kotaro Kohno,A. Labiano,Georgios E. Magdis,Matthew A. Malkan,Hideo Matsuhara,Tohru Nagao,David A. Naylor,Miguel Pereira-Santaella,Francesca Pozzi,Giulia Rodighiero,Peter Roelfsema,Stephen Serjeant,Cristian Vignali,Lingyu Wang,Toru Yamada +33 more
TL;DR: In this article, the authors use the SPACE Infrared telescope for Cosmology and Astrophysics (SPICA) project as a template to demonstrate how deep spectrophotometric surveys covering large cosmological volumes over extended fields (1-15 deg2) with a mid-IR imaging spectrometer (17-36 μm) in conjunction with deep 70 μm photometry with a far-IR camera, at wavelengths which are not affected by dust extinction can answer the most crucial questions in current galaxy evolution studies.
Galaxy evolution through infrared and submillimetre spectroscopy: Measuring star formation and black hole accretion with JWST and ALMA
TL;DR: In this article , the spectral lines and features that can be detected by JWST-MIRI in galaxies and active galactic nuclei up to redshift up to 3.5 GHz were used to measure the Star Formation (SF) and the Black Hole Accretion (BHA) rates.
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Calibration of mid- to far-infrared spectral lines in galaxies
TL;DR: In this paper, the authors derived robust star-formation tracers based on the [CII]158$\mu$m line; the sum of the [OI]63$/m and [OIII]88$ /m lines; a combination of the neon and sulfur mid-IR lines; the bright PAH features at 6.2 and 11.3
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The physics of galaxy evolution with SPICA observations
Luigi Spinoglio,J. A. Fernández-Ontiveros,Sabrina Mordini +2 more
- 01 Mar 2020
TL;DR: The Space Infrared Telescope for Cosmology and Astrophysics (SPICA) as discussed by the authors was designed for the 5th Medium Size ESA Cosmic Vision Mission (SVM) with its 2.5m mirror cooled down to T < 8K.
The physics of Galaxy Evolution with SPICA observations
TL;DR: The future IR space telescope mission, SPICA, currently under evaluation for the 5th Medium Size ESA Cosmic Vision Mission, fully redesigned with its 2.5 m mirror cooled down to T < 8K, will provide for the first time a 3D spectroscopic view of the hidden side of star formation and black hole accretion in all environments, from voids to cluster cores over 90% of cosmic time.