User Tools

Site Tools


ao:acq_system

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
ao:acq_system [2018/07/07 08:31]
jones [Camera Selection]
ao:acq_system [2018/07/07 08:33] (current)
jones [Acquisition System]
Line 1: Line 1:
-====== Acquisition System ======+====== Acq System ======
  
 ==== Optical Layout ==== ==== Optical Layout ====
Line 10: Line 10:
 ==== Camera Selection ==== ==== Camera Selection ====
 \\   \\  
-An ideal acquisition camera should enable both fast and slow readout, with dark current lower than typical sky noise. The current acquisition camera is a camera with a BNC connector made by Watec (the 120N?). The short axis of the field of view is 5.7mm (? to confirm). An alternative camera is the (uncooled) [[http://www.astronomycameras.com/products/usb/dmk41au02as/|DMK.AU02]]CCD camera from Imaging Source. This has a short axis of 4.76mm, and a diagonal of 7.96mm. The CCD datasheet for this larger format sensor is [[/here|here]], and the more sensitive and smaller version MJI is familiar with is [[/here|here]]. This smaller version has definitely been seen to be sky noise limited (i.e. not dark or readout noise) for ~1 sec exposures. Gig-E versions are available.\\ +An ideal acquisition camera should enable both fast and slow readout, with dark current lower than typical sky noise. The current acquisition camera is a camera with a BNC connector made by Watec (the 120N?). The short axis of the field of view is 5.7mm (? to confirm). An alternative camera is the (uncooled) [[http://www.astronomycameras.com/products/usb/dmk41au02as/|DMK.AU02]]CCD camera from Imaging Source. This has a short axis of 4.76mm, and a diagonal of 7.96mm. The CCD datasheet for this larger format sensor is [[ao:here|here]], and the more sensitive and smaller version MJI is familiar with is [[ao:here|here]]. This smaller version has definitely been seen to be sky noise limited (i.e. not dark or readout noise) for ~1 sec exposures. Gig-E versions are available.\\ 
 \\  \\ 
 //Laszlo:// Currently we use Astrovid Stellacam II video cameras for both imege acquisition and for the finder. This camera looks very much like a Watec camera only a bit larger. I suspect it is made by Watec. The Astrovid uses Sony ICX418AL CCD while the DMK camera uses Sony ICX205AL CCD. Both CCDs are Type 1/2, that is 8 mm diagonally. According to the datasheets the sensitivity of the ICX418AL and ICX205AL are 1100 mV and 450 mV, respectively. The Astrovid dark signal is 1 mV while the DMK dark signal is 16 mV. Thus the Astrovid is more sensitive than the DMK. The Astrovid has an analog output and needs a frame grabber. This is not ideal. It would be nice to have digital output. The USB output of the DMK is not ideal either because we either use the WFS computer to handle the acquisition finder cameras or we need a bunch of repeaters because USB 2 is limited to 5 m cable length and the bunkers are rather 30 m away.\\   //Laszlo:// Currently we use Astrovid Stellacam II video cameras for both imege acquisition and for the finder. This camera looks very much like a Watec camera only a bit larger. I suspect it is made by Watec. The Astrovid uses Sony ICX418AL CCD while the DMK camera uses Sony ICX205AL CCD. Both CCDs are Type 1/2, that is 8 mm diagonally. According to the datasheets the sensitivity of the ICX418AL and ICX205AL are 1100 mV and 450 mV, respectively. The Astrovid dark signal is 1 mV while the DMK dark signal is 16 mV. Thus the Astrovid is more sensitive than the DMK. The Astrovid has an analog output and needs a frame grabber. This is not ideal. It would be nice to have digital output. The USB output of the DMK is not ideal either because we either use the WFS computer to handle the acquisition finder cameras or we need a bunch of repeaters because USB 2 is limited to 5 m cable length and the bunkers are rather 30 m away.\\  
ao/acq_system.1530966713.txt.gz ยท Last modified: 2018/07/07 08:31 by jones