Fabrizio Cogato
A5092829132- Astronomy and Astrophysical Research
- Gamma-ray bursts and supernovae
- Infrared Target Detection Methodologies
- Cosmology and Gravitation Theories
- Sensor Technology and Measurement Systems
- Galaxies: Formation, Evolution, Phenomena
- Calibration and Measurement Techniques
- Spacecraft Design and Technology
- Historical Astronomy and Related Studies
- Inertial Sensor and Navigation
- Advanced Semiconductor Detectors and Materials
- Remote-Sensing Image Classification
- Remote Sensing in Agriculture
- Satellite Image Processing and Photogrammetry
- Industrial Vision Systems and Defect Detection
- Stellar, planetary, and galactic studies
- Scientific Research and Discoveries
- Biblical Studies and Interpretation
- Historical and Architectural Studies
- Spectroscopy and Laser Applications
Aix-Marseille Université
2024
Osservatorio di Astrofisica e Scienza dello Spazio
2023-2024
National Institute for Astrophysics
2024
University of Bologna
2023
The Near-Infrared Spectrometer and Photometer (NISP) on board the Euclid satellite provides multiband photometry R>=450 slitless grism spectroscopy in 950-2020nm wavelength range. In this reference article we illuminate background of NISP's functional calibration requirements, describe instrument's integral components, provide all its key properties. We also sketch processes needed to understand how NISP operates is calibrated, technical potentials limitations. Links articles providing more...
PLATO (PLAnetary Transits and Oscillations of stars) is an M3 medium-class space mission in ESA's Cosmic Vision program devoted to detecting studying a large number extrasolar planetary systems. Its launch planned for the end 2026 from Europe's Spaceport French Guiana. The Payload consists 26 wide field-of-view Cameras, each observing specific part sky, associated data processing units power supply units. 24 Normal-Cameras will provide very high-resolution photometric measurement light...
ABSTRACT Combining cosmological probes has consolidated the standard model with per cent precision, but some tensions have recently emerged when certain parameters are estimated from local or primordial Universe. The origin of this behaviour is still under debate; however, it crucial to study as many possible cross-check results independent methods and provide additional pieces information puzzle. In work, by combining several late-Universe (0 < z 10), namely, Type Ia supernovae,...
PLATO (PLAnetary Transits and Oscillations of stars)1 is the M3 class ESA mission dedicated to discovery study extrasolar planetary systems by means transits detection. Payload Camera units are integrated vibrated at CSL before being TVAC tested for thermal acceptance performance verification 3 different test facilities (SRON, IAS INTA). 15 26 Flight Cameras were integrated, delivered integration Prime between June 2023 2024, with remaining flight be end 2024. In this paper, we provide an...
Launched successfully on July 1st, 2023, Euclid, the M2 mission of ESA cosmic vision program, aims mainly at understanding origin accelerated expansion Universe. Along with a visible imager VIS, it is equipped NISP instrument, Near Infrared Spectrometer and Photometer, bespoke tailored to perform 3D mapping observable It operates in near-infrared spectral range, from 900 nm 2000 2 observing modes: as spectrometer, instrument will permit measuring millions galaxy spectroscopic redshifts over...
Combining cosmological probes has consolidated the standard model with percent precision, but some tensions have recently emerged when certain parameters are estimated from local or primordial Universe. The origin of this behaviour is still under debate, however, it crucial to study as many possible cross-check results independent methods and provide additional pieces information puzzle. In work, by combining several late-Universe (0$<z<$10), namely, Type Ia SuperNovae, Baryon Acoustic...