21 July 2010 Analysis of LBT LINC-NIRVANA simulated images of galaxies
Author Affiliations +
Abstract
LINC-NIRVANA (LN) is a Fizeau interferometer that will provide coherent images in the near-IR combining the beams from the two Large Binocular Telescope (LBT) arms, by adopting a Multi-Conjugate Adaptive Optics system (MCAO) that allows for atmospheric turbulence compensation. We applied the software AIRY-LN for the simulation and the reconstruction of LN images in order to investigate the dependence of the image quality from the magnitude of the star used for the PSF extraction. A good knowledge of this dependence is a crucial point for the LN observations, especially for the extragalactic target where the presence of a bright psf-star within the LN field of view of 10×10 arcsec is not granted. Our results, although still preliminary, show that while from the morphological point of view the use of psf-star up to a magnitude of 18 is still acceptable, from the photometric point of view the use of psf-star fainter than Ks ~ 16 mag could cause considerable problems.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Paolo Ciliegi, Andrea La Camera, Carmelo Arcidiacono, Mario Bertero, Patrizia Boccacci, Emiliano Diolaiti, Italo Foppiani, Matteo Lombini, Laura Schreiber, "Analysis of LBT LINC-NIRVANA simulated images of galaxies", Proc. SPIE 7734, Optical and Infrared Interferometry II, 77342G (21 July 2010); doi: 10.1117/12.856951; https://doi.org/10.1117/12.856951
PROCEEDINGS
10 PAGES


SHARE
RELATED CONTENT

Steller populations in the nearby universe
Proceedings of SPIE (December 16 2002)
Data fusion and photometric restoration
Proceedings of SPIE (November 01 2001)
Tests of the PSF reconstruction algorithm for NACO/VLT
Proceedings of SPIE (July 16 2008)
ONIRICA an infrared camera for OWL with MCAO low...
Proceedings of SPIE (June 27 2006)

Back to Top