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Physics

D-Index
95
Citations
32530
World Ranking
1933
National Ranking
101

Overview

Paolo Ciliegi is affiliated with the National Institute for Astrophysics in Italy. Their research primarily spans the intersecting fields of Physics and Astronomy and Engineering, with a considerable focus on subfields including Atomic and Molecular Physics, and Optics, Electrical and Electronic Engineering, Instrumentation, Astronomy and Astrophysics, and Biomedical Engineering.

The main topics of Paolo Ciliegi's work cover Adaptive Optics and Wavefront Sensing, Optical Systems and Laser Technology, Astronomy and Astrophysical Research, Advanced Optical System Design, Stellar, Planetary, and Galactic Studies, Calibration and Measurement Techniques, and Radio Astronomy Observations and Technology.

They have contributed significantly to scholarly publications across multiple venues. Frequent publication venues include Adaptive Optics Systems VIII, arXiv (Cornell University), Ground-based and Airborne Instrumentation for Astronomy IX, Astronomy and Astrophysics, and the Journal of Astronomical Telescopes Instruments and Systems.

  • MAORY/MORFEO@ELT: general overview up to the preliminary design and a look towards the final design (2022, Adaptive Optics Systems VIII)
  • LOFAR HBA observations of the Euclid Deep Field North (EDFN) (2024, Astronomy and Astrophysics)
  • Mechanical design overview for the main structure of MAORY/MORFEO (2022, Ground-based and Airborne Instrumentation for Astronomy IX)
  • MAORY: A Multi-conjugate Adaptive Optics RelaY for ELT (2021, arXiv (Cornell University))
  • MORFEO optical design and performances: status at preliminary design review (2022, Adaptive Optics Systems VIII)

Paolo Ciliegi regularly collaborates with other researchers. Frequent co-authors include Lorenzo Busoni, Guido Agapito, Marco Riva, Demetrio Magrin, and Cédric Plantet. These collaborations suggest a strong network within the domain of adaptive optics and related instrumentation.

Best Publications

  • Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey

    O. Ilbert;S. Arnouts;H.J. McCracken;M. Bolzonella

  • Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey

    O. Ilbert;O. Ilbert;S. Arnouts;H. J. Mccracken;M. Bolzonella

  • zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field

    S.J. Lilly;O. Le Fevre;A. Renzini;G. Zamorani

  • zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 < z < 3 in the COSMOS Field*

    S. J. Lilly;O. Le Fèvre;A. Renzini;G. Zamorani

  • The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5<=IAB<=24, and the redshift distribution over 0< z <=5

    O. Le Fevre;G. Vettolani;B. Garilli;L. Tresse

  • A test of the nature of cosmic acceleration using galaxy redshift distortions

    L. Guzzo;M. Pierleoni;B. Meneux;E. Branchini

  • The Universe as Seen by ISO

    M. Rowan-Robinson;S. Oliver;A. Efstathiou;C. Gruppioni

  • The VIMOS VLT deep survey. First epoch VVDS-deep survey: 11 564 spectra with 17.5 ≤ IAB ≤ 24, and the redshift distribution over 0 ≤ z ≤ 5

    O. Le Fèvre;G. Vettolani;B. Garilli;L. Tresse

  • The HELLAS2XMM survey. VII. The hard X-ray luminosity function of AGN up to z=4: more absorbed AGN at low luminosities and high redshifts

    F. La Franca;F. Fiore;A. Comastri;G.C. Perola

  • The HELLAS2XMM Survey. VII. The Hard X-Ray Luminosity Function of AGNs up to z = 4: More Absorbed AGNs at Low Luminosities and High Redshifts

    F. La Franca;F. Fiore;A. Comastri;G. C. Perola

  • The VIMOS VLT Deep Survey: Public release of 1599 redshifts to IAB<=24 across the Chandra Deep Field South

    O. Le Fevre;G. Vettolani;S. Paltani;L. Tresse

  • The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z~6.7 selected with 17.5<=i_{AB}<=24.7

    O. Le Fevre;P. Cassata;O. Cucciati;B. Garilli

  • The SWIRE-VVDS-CFHTLS surveys: stellar mass assembly over the last 10 Gyears. Evidence for a major build up of the red sequence between z=2 and z=1

    S. Arnouts;C.J. Walcher;O. Le Fevre;G. Zamorani

  • The VLA-COSMOS Survey. II. Source Catalog of the Large Project

    E. Schinnerer;V. Smolčić;C. L. Carilli;M. Bondi

  • The VIMOS-VLT Deep Survey: Evolution of the galaxy luminosity function up to z=2 in first epoch data

    O. Ilbert;L. Tresse;E. Zucca;S. Bardelli

  • The Vimos VLT deep survey - stellar mass segregation and large-scale galaxy environment in the redshift range 0.2 < z < 1.4

    M. Scodeggio;D. Vergani;D. Vergani;O. Cucciati;O. Cucciati;A. Iovino

  • EMU: Evolutionary Map of the Universe

    Ray P. Norris;Andrew M. Hopkins;Andrew M. Hopkins;Jose Afonso;S. Brown

  • The HELLAS2XMM survey IV. Optical identifications and the evolution of the accretion luminosity in the Universe

    F. Fiore;M. Brusa;M. Brusa;F. Cocchia;F. Cocchia;A. Baldi

  • The SWIRE-VVDS-CFHTLS surveys: stellar mass assembly over the last 10 Gyr. Evidence for a major build up of the red sequence between z = 2 and z = 1

    S. Arnouts;C. J. Walcher;O. Le Fèvre;G. Zamorani

  • The VIMOS VLT Deep Survey. Public release of 1599 redshifts to I AB ≤24 across the Chandra Deep Field South

    O. Le Fevre;G. Vettolani;S. Paltani;L. Tresse

Frequent Co-Authors

H. J. McCracken
H. J. McCracken Institut d'Astrophysique de Paris
S. Bardelli
S. Bardelli National Institute for Astrophysics
Lucia Pozzetti
Lucia Pozzetti National Institute for Astrophysics
A. Iovino
A. Iovino National Institute for Astrophysics
A. Cappi
A. Cappi National Institute for Astrophysics
O. Le Fevre
O. Le Fevre Aix-Marseille University
Luigi Guzzo
Luigi Guzzo University of Milan
Elena Zucca
Elena Zucca National Institute for Astrophysics
G. Zamorani
G. Zamorani National Institute for Astrophysics
D. Maccagni
D. Maccagni National Institute for Astrophysics

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