TEIGA Logo

Andrea La Camera's personal page

Remark: This page is an updated version of my previous homepage at DIBRIS. Here you can find the publications and the software for the deconvolution of astronomical images.

More info: Google Scholar |  ADS Nasa |  SPIE.org |   Research Gate

Publications

49 publications:Chapter of Books (1) Articles (18) Proceedings (28) Other (2)
Group by:

Chapter of Books 1

Articles 18

Proceedings 28

Other 2

  • Deblurring of post-adaptive optics images

    Andrea La Camera & Laura Schreiber

    SPIE Newsroom·2015

    Other
  • Simulation and reconstruction of LBT LINC-NIRVANA images: two specific science cases

    Paolo Ciliegi, Emiliano Diolaiti, Matteo Lombini, Filippo Mannucci, Massimo Salvati, Carmelo Arcidiacono, Mario Bertero, Patrizia Boccacci, Gabriele Desiderà, Andrea La Camera, Simone Antoniucci, Dario Lorenzetti & Brunella Nisini

    2008

    Other

Software

1 - Software Package AIRY

AIRY logo

The Software Package AIRY (Astronomical Image Restoration in interferometrY) is oriented to the reconstruction of interferometric images and it is also applicable to the case of a single dish telescope.
It can be used both for the reconstruction and for the simulation of astronomical images. AIRY is written in IDL and must be used together with the CAOS Application Builder.

Both AIRY and CAOS are downloadable for free here.

2 - Software Package AIRY-LN

AIRY-LN logo

The Software Package AIRY-LN is developed for LINC-NIRVANA (LN), the interferometric camera of the Large Binocular Telescope (LBT) and it is oriented to the reconstruction of the LN images. It can be used in a simulation program for reconstructing images generated by means of AIRY.

3 - PATCH

PATCH logo

The Software PATCH is a tool for the deblurring of post-AO images characterized by space-variant PSFs. It is based on the assumption that the PSF smoothly varies across the image domain. The image is decomposed into sub-domains (or “patches”), then each sub-domain is separately reconstructed by means of a deconvolution method and the final image is obtained as a mosaic of the results. More information can be found on the SPIE Newsroom webpage as well as on this GitLab page.

Last update: 2026-07-24.
Please send suggestions and comments to andrea[at]teiga.it