# SI 1100S

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## Spectral Instruments 1100S CCD

This CCD camera is currently the main imaging instrument on the RCC telescope.

An SI 1100S camera with Johnson-Cousins B,V,R,I and Sloan u,g,r,i,z filters is currently mounted on the telescope yielding an approximately 16'x16' FoV. Camera control is implemented via ccdsh after the camera drivers are loaded. This can be done with the following command:

source /usr/local/ccdsh/scripts/load-ace-sicamera.ccdsh


This line can also be included in the user's local startup script in the home directory. The camera driver file contains the followings:

module mod_sicamera.so
module mod_ace_filter.so

define  filter  1       B       "Bessel B"
define  filter  2       V       "Bessel V"
define  filter  3       R       "Bessel R"
define  filter  4       I       "Bessel I"
define  filter  5       C       "Clear"
define  filter  6       u       "Sloan u"
define  filter  7       g       "Sloan g"
define  filter  8       r       "Sloan r"
define  filter  9       i       "Sloan i"
define  filter  10      z       "Sloan z"
define  filter  11      E       "Empty"



The first two lines load the camera and filter modules respectively, and the next eleven defines the filters.

### Parameters

The basic parameters of the camera and its CCD are the following:

• Resolution: 4096 x 4096
• Pixel size: 15 x 15 microns
• Effective field-of-view: 16 x 16 arcminutes
• Effective resolution: 0.23"/pixel
• Available binning modes: 1x1
• Gain: ~2.63 (depends on the channel)

### Filters

The third column of the driver file contains the filter positions, the fourth the names which the filter can be referred to when using the set filter command, and the fifth contains the names.

### Notes

• Camera readout is done via four channels. The gain and readnoise values are slighlty different for the four channel. Please see the quality test report below for details!
• The camera can be cooled to $-115^{\circ}\mathrm{C}$ via crycooling. The cooler should operate all the time. In case of temperature increase there is a vacuum loss, which renders the camera unoperable! Please always check the camera temperature! The operating vacuum is around 0.002-0.003 torr. You can check this in the fits header, under PARAM7.
• The pickoff mirror and the off-axis guider mirrors block the light from reaching the camera. Do not forget to switch off the spectrograph: acectrl --stop, and move the guider mirror to the side: acectrl --guide-xstage-reset, before starting the observations.
• The camera can be focused with the usual set focus command within ccdsh.
• For quality test, see this document:File:1100-189 TestReport-RMA-6112-Data-.pdf
• Currently (2019.08.28), the ccdsh module for the camera does NOT support trimming and binning. Please do not attempt to use trimming or binning until further notice!
• Currently (2019.08.28), both the ccdsh module and the windows backend does NOT support image interruption. Therefore, it is advised to insert a delay=1 or delay=2 into each image definitions within the ccdsh sequence, for instance sequence -n dark 10*[dark,20,delay=2] and then interrupt the sequence (with Ctrl+C) while the system is delaying there -- in this example, for 2 seconds.
• You can check the status of the windows program which currently operating the camera here: vncviewer 172.31.171.171. Please do not modify anything here!

### How to observe with the camera

Usage of the SI 1100S on the RCC