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GMOS-S Array (Hamamatsu)

The upgraded GMOS-S detector array consists of three ~ 2048x4176 Hamamatsu chips arranged in a row. Two of the detectors (CCDr and CCDg) have an enhanced red response, these CCDs are referred to by the ITC as "Hamamatsu Red". The right-most CCD (CCDb, the blue end of spectral dispersion dispersion) in the focal plane array has improved blue response in addition to red response very similar to the Hamamatsu Red CCDs. This third CCD is referred to by the ITC as "Hamamatsu Blue". The orientation of the CCDs will remain unchanged and will continue to support the Nod and Shuffle observing mode. The plot below gives the anticipated QE comparison to the current E2V CCDs in GMOS-S. These QE plots are taken from general Hamamatsu information and lab measurements done in Hilo. See the Status and Availability webpage for more details.

 

 
QE Comparison for the GMOS-S CCDs upgrade. 

 

The table below summarizes some of the expected Hamamatsu detector/controller characteristics.

Array Hamamatsu
Pixel format 6266x4176 pixels (mosaiced)
Array layout Three 2048x4176 chips in a row with 61pix=0.915mm gaps
Pixel size 15 microns square; 0.080 arcsec/pixel
Spectral Response approx 0.36 to 1.03 microns [ Hamamatsu Red data / Hamamatsu Blue data / plot ]
Bias level Bias Image
Flat field response not yet available
Readout time 1x1: 83sec(slow)/35sec(fast)   2x2: 25sec(slow)/16sec(fast)
Chip CCDr CCDg CCDb
Chip ref no. BI5-36-4k-2 BI11-33-4k-1 BI12-34-4k-1
Dark current ~ 3e-/hr/pix ~ 3e-/hr/pix ~ 3e-/hr/pix
Full Well ~110,000 e- ~110,000 e- ~100,000 e-
Fringing at 900nm <2% <2% <2%

 

 

Readnoise and Gain Values

The table below gives gain/read-noise values for the new GMOS Hamamatsu CCDs operating with the SDSU controller. The values are averaged over all 12 amps.  

 

Readout Gain Resulting average
rate level Gain (e-/ADU) noise (e- rms)
Slow Low 1.64 3.82
Fast High 1.41 5.55
Fast Low 5.14 7.67

 

The Slow Read / High Gain mode will not be offered for the Hamamatsu CCDs as it has been deemed to be of little scientific use. Slow Read / Low Gain is the primary mode for science use. Fast Read / Low Gain may be of use, for example, with acquisition observations or for time resolved observations. Fast Read / High Gain is expected to be used primarily for very bright targets.

The linearity is better than ~1% up to 60k as shown by preliminary results.

The cosmic ray hit rate is higher on the Hamamatsu CCDs - about twice that of the older EEVs.