The CAMCAO infrared camera
- Author(s)
- Antonio Amorim, Antonio Melo, Joao Alves, Jose Rebordao, Jose Pinhao, Gregoire Bonfait, Jorge Lima, Rui Barros, Rui Fernandes, Isabel Catarino, Marta Carvalho, Rui Marques, Jean-Marc Poncet, Filipe Duarte Santos, Gert Finger, Norbert Hubin, Gotthard Huster, Franz Koch, Jean-Louis Lizon, Enrico Marchetti
- Abstract
The CAMCAO instrument is a high resolution near infrared (NIR) camera
conceived to operate together with the new ESO Multi-conjugate Adaptive
optics Demonstrator (MAD) with the goal of evaluating the feasibility of
Multi-Conjugate Adaptive Optics techniques (MCAO) on the sky. It is a
high-resolution wide field of view (FoV) camera that is optimized to use
the extended correction of the atmospheric turbulence provided by MCAO.
While the first purpose of this camera is the sky observation, in the
MAD setup, to validate the MCAO technology, in a second phase, the
CAMCAO camera is planned to attach directly to the VLT for scientific
astrophysical studies. The camera is based on the 2kx2k HAWAII2 infrared
detector controlled by an ESO external IRACE system and includes
standard IR band filters mounted on a positional filter wheel. The
CAMCAO design requires that the optical components and the IR detector
should be kept at low temperatures in order to avoid emitting radiation
and lower detector noise in the region analysis. The cryogenic system
inclues a LN2 tank and a sptially developed pulse tube cryocooler. Field
and pupil cold stops are implemented to reduce the infrared background
and the stray-light. The CAMCAO optics provide diffraction limited
performance down to J Band, but the detector sampling fulfills the
Nyquist criterion for the K band (2.2mm).
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Universidade de Coimbra, European Southern Observatory (Germany), Universidade de Lisboa, National Institute of Engineering, Technology and Innovation (INETI), Universidade Nova de Lisboa
- Journal
- Proceedings of SPIE
- Volume
- 5492
- Pages
- 1699-1709
- ISSN
- 0277-786X
- DOI
- https://doi.org/10.1117/12.549008
- Publication date
- 09-2004
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103004 Astrophysics
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/7d06020b-f149-469a-8cd4-75282403fcb6