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First optical elements

Last October we received the first optical elements, the uncoated mirrors.

Order of Optic and Cryostat

On May 2009, the Optic was ordered to SESO. And at the same time, the cryostat was also ordered to Reuter.

We hope the optic will be delivered in one year.

Cryostat

Realistic images of the lastes design with carbon fiber adapter. See images here.


Welcome to the PANIC Project website

PANIC is the new PAnoramic Near-Infrared Camera for the 2.2m telescope on Calar Alto Observatory. The project started in September 2006. It is a joint project between MPIA (Max-Planck-Institut für Astronomie ) and IAA (Instituto de Astronomia de Andalucia in Granada).

The aim of the project is to build a wide-field general purpose NIR camera. Of course it will be very well suited for surveys.

With its focal plane array of 2x2 HAWAII2-RG detectors it covers a 30x30 arcmin field-of-view and it has a pixel scale of 0.45 arcsec/pixel. The cryogenic optics has three flat folding mirrors with diameters up to 270 mm and eight lenses with diameters between 115 mm and 250 mm. A compact filter unit can carry up to 19 filters distribited over four filter wheels. The wheels have cryogenic stepper motors.
The instrument has a diameter of 1.1 m and it is about 1 m long. Since the there is a weight limit of only 400 kg at the 2.2 m telescope, a lightweight cryostat design is necessary. The aluminium vacuum vessel and radiation shield have wall thicknesses of only 6 mm and 3 mm respectively. Cooling is done by liquid nitrogen.



PANIC in a Nutshell

Telescope

Cassegrain 2.2m Calar Alto

F Ratio

f/8

Field of view

30' x 30'

Direct Imagin

Over the whole FOV

Pixel scale

0.45 arcsec/pixel

Detector

2 x 2 mosaic of 4 Hawaii-2 RG

Gap between detectors

167 pìxels

Filling factor

98%

Wavelength range

0.95– 2.45 mm with IQ

0.82-0.95 mm able to transmit

Filters

Broad band ZYJHK

Narrow band: ~1%

Intrinsic image quality

EE80 <= 2 pixels = 0.9 arcsec=36 mm

Pupil Image available

Cold stop

Geometrical distortions

<= 1.5%

Operating temperature

80K (liquid nitrogen)

Data format

FITS




PANIC Collaboration

PANIC is a collaborative effort of these institutions:

Science

We list below potential scientific cases that would benefit from the panoramic imaging mode of PANIC. More details for some of them can be found in the Phase A document, section 2. A (non-exhaustive) compilation of science cases that would benefit from the other TBC observing modes is also given.

PANIC Team

The following people form the PANIC team:

Workpackages

The workpackages involved in PANIC development are:

Gallery

Here you can find some astronomical images, photographs, animations and videos concerning PANIC

News

Here you can find the latest news on PANIC project.

Links

Some usefull links:

Contact us

If you have any question or suggestion about PANIC project, please feel free to contact us.

Downloads

This folder has some documents to download by external and internal users.