[图书][B] Polarized light and optical systems

R Chipman, WST Lam, G Young - 2018 - taylorfrancis.com
Polarized Light and Optical Systems presents polarization optics for undergraduate and
graduate students in a way which makes classroom teaching relevant to current issues in …

[图书][B] Thin-film optical filters

HA Macleod, HA Macleod - 2010 - taylorfrancis.com
Written by a world-renowned authority of optical coatings, Thin-Film Optical Filters, Fourth
Edition presents an introduction to thin-film optical filters for both manufacturers and users …

[HTML][HTML] Point spread function modelling for astronomical telescopes: a review focused on weak gravitational lensing studies

TI Liaudat, JL Starck, M Kilbinger - Frontiers in Astronomy and Space …, 2023 - frontiersin.org
The accurate modelling of the point spread function (PSF) is of paramount importance in
astronomical observations, as it allows for the correction of distortions and blurring caused …

About the effects of polarising optics on lidar signals and the Δ90 calibration

V Freudenthaler - Atmospheric Measurement Techniques, 2016 - amt.copernicus.org
This paper provides a model for assessing the effects of polarising optics on the signals of
typical lidar systems, which is based on the description of the individual optical elements of …

Polarization aberrations in next-generation giant segmented mirror telescopes (GSMTs)-I. Effect on the coronagraphic performance

RM Anche, JN Ashcraft, SY Haffert… - Astronomy & …, 2023 - aanda.org
Context. Next-generation large segmented mirror telescopes are expected to perform direct
imaging and characterization of Earth-like rocky planets, which requires contrast limits of …

Numerical modeling of the proposed WFIRST-AFTA coronagraphs and their predicted performances

J Krist, B Nemati, B Mennesson - Journal of Astronomical …, 2016 - spiedigitallibrary.org
The WFIRST-AFTA 2.37 m telescope will provide the opportunity to host a coronagraph for
the imaging and spectroscopy of planets and disks in the next decade. The telescope …

Sphere/zimpol high resolution polarimetric imager-i. system overview, psf parameters, coronagraphy, and polarimetry

HM Schmid, A Bazzon, R Roelfsema, D Mouillet… - Astronomy & …, 2018 - aanda.org
Context. The SPHERE “planet finder” is an extreme adaptive optics (AO) instrument for high
resolution and high contrast observations at the Very Large Telescope (VLT). We describe …

Satellite-relayed global quantum communication without quantum memory

S Goswami, S Dhara - Physical Review Applied, 2023 - APS
Photon loss is the fundamental issue toward the development of quantum networks. To
circumvent loss quantum repeaters were proposed, which need high-performance quantum …

The speckle polarimeter of the 2.5-m telescope: Design and calibration

BS Safonov, PA Lysenko, AV Dodin - Astronomy Letters, 2017 - Springer
The speckle polarimeter is a facility instrument of the 2.5-mSAIMSU telescope that combines
the features of a speckle interferometer and a polarimeter. The speckle polarimeter is …

Vectorial adaptive optics

C He, J Antonello, MJ Booth - eLight, 2023 - Springer
Adaptive optics normally concerns the feedback correction of phase aberrations. Such
correction has been of benefit in various optical systems, with applications ranging in scale …