PANIC: current status

We will present the current status of the PANIC project. This instrument will be the first to be built inside the Spanish-German consortium signed between MPIA and IAA for the development of new instrumentation for the Calar Alto Observatory. PANIC is a wide-field infrared imager for the Ritchey-Chrétien focus of the Calar Alto 2.2m and 3.5m telescopes. The camera optical design is a folded single optical train that images the sky onto the focal plane with a plate scale of 0.45" per 18 µm pixel at the 2.2m and 0.23"/px at the 3.5m. A mosaic of four Hawaii 2RG of 2k x 2k made by Teledyne, will give a field of view of 31.9 arcmin x 31.9 arcmin and 16.4 arcmin x 16.4 arcmin, respectively. This cryogenic instrument will cover the photometric bands from Z to K (0.8 to 2.5 µm). The control software of the instrument can be divided into the GEIRS for the basic control, and a tool for support the observation, the Observing Tool. Regarding the data handling, PANIC will have a Quick-Look tool for pre-reduction and visualization of the raw data, and a pipeline for the complete reduction.

In this talk, we will outline the main features and the present status of these software components and some examples already implemented will be given.

 

Fecha: 
29/10/2009 - 13:00
Conferenciante: 
Matilde Fernández, Julio F. Rodríguez, Conchi Cárdenas y José M. Ibáñez
Filiación: 
Instituto de Astrofísica de Andalucía - CSIC


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