Paolo Madonia

ORCID: 0000-0003-2495-0724
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About
Contact & Profiles
Research Areas
  • Superconducting and THz Device Technology
  • Gamma-ray bursts and supernovae
  • Laser-induced spectroscopy and plasma
  • Geomagnetism and Paleomagnetism Studies
  • Microwave Engineering and Waveguides
  • Physics of Superconductivity and Magnetism
  • Advanced Thermodynamic Systems and Engines
  • Stellar, planetary, and galactic studies
  • Astrophysics and Star Formation Studies
  • Galaxies: Formation, Evolution, Phenomena
  • Nuclear Physics and Applications
  • Scientific Research and Discoveries
  • Calibration and Measurement Techniques

California Institute of Technology
2020-2021

Sapienza University of Rome
2020

Line intensity mapping (LIM) provides a unique and powerful means to probe cosmic structures by measuring the aggregate line emission from all galaxies across redshift. The method is complementary conventional galaxy redshift surveys that are object-based demand exquisite point-source sensitivity. Tomographic Ionized-carbon Mapping Experiment (TIME) will measure star formation rate (SFR) during reionization observing redshifted [CII] 158$\mu$m ($6 \lesssim z 9$) in LIM regime. TIME...

10.3847/1538-4357/abfe62 article EN The Astrophysical Journal 2021-07-01

TIME is an instrument being developed to study emission from faint objects in our universe using line intensity mapping (LIM) understand the over cosmic time. The a mm-wavelength grating spectrometer with Transition Edge Sensor (TES) bolometers measuring frequency range of 200-300 GHz 60 spectral pixels and 16 spatial pixels. will measure [CII] redshift 5 9 probe evolution during epoch reionization. also low-redshift CO fluctuations map molecular gas peak star formation 0.5 2. This emerging...

10.1117/12.2561865 article EN 2020-12-12
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