MIKE CCD system

Each MIKE CCD detector system uses a 2K × 4K back-illuminated device, with 15 µm pixels and two output amplifiers.  At present, the red channel uses a SITe ST-002A CCD, while the blue channel uses a MIT Lincoln Labs CCID-20.  The ST-002A has a standard broadband AR coating.  The CCID-20 has a blue enhanced coating.  Each detector is mounted in a rectangular aluminum housing.  The dewar window on each side is the field flattener of the camera.

The CCD housing is coupled to an IR-Labs ND-5 cryostat, with the CCD control electronics box attached to the side of the dewar (see photo).  Each CCD is liquid nitrogen cooled and has roughly 15 hour hold time in the horizontal position.  Inside the housing, the CCD is connnected to a rigid-flex preamp board, which brings the signals out on a flex cable to a hermetic connector.

Each CCD controller is a compact dual-channel digital signal processor based system, capable of both high-speed and slow-scan readout.  We plan to operate in slow-scan mode, using only the better of the two CCD output amplifiers for the lowest noise performance.  Lab tests show that read noise is  about 4 e-/pixel for the SITe device.  The LL device has a measured read noise of 1.8 e-.  The two detector systems are mounted side-by-side on the instrument (see photo) and operate independently.  That is, they have independent shutters,  exposure times and readout times.

[from R. Bernstein et al, "MIKE: A double-echelle spectrograph for the Magellan telescopes at Las Campanas Observatory,"  SPIE 4841 Astronomical Telescopes and Instrumentation, Kona (2002).]


CCD Properties

CCD Detector Properties
Device Specifications ST-002A
CCID-20
Units
Peak Quantum Efficiency >80 >90
%
Array size 2048 × 4096
2048 × 4096
pixels
Pixel size 15
15
µm
Amplifiers 2 2

Full well
>60
20
ke-
Dark current (at -125 °C)
< 1
3.6
e-/hr
Spurious charge 0.2 0.35 e-


CCD Quantum efficiency measurements

MIKE red ccd QE curve -- from SITe test documentation


MIKE blue ccd QE curve -- measured.  Note the QE calibration is off at short wavelengths, where the measurement exceeds 100%.



Dewar Mechanical Internals

The CCD housing for the MIKE detectors is machined from a block of aluminum, and measures  6.625 inches x 6.625 inches x 5 inches deep (see mechanical drawings).

The MIKE_RED ccd is mounted on an Invar package by SITe, and has a 3 inch ribbon cable to connect the electrical signals.  The ribbon cable terminates in a 40-pin RN plastic connector.  The ribbon cable is not thermally isolating, so we have a 2-inch flex cable which connects the ccd ribbon cable to the 37-pin preamp connector.

The MIKE_BLUE ccd is mounted on an AlN substrate, and has a short flex cable for the ccd signals. The flex cable terminates in a 37-pin micro-D connector.  A short cross-connect cable of constantan wire connects the ccd flex-cable to the preamp connector.

We mount both the SITe package and the LL package onto a small Invar substrate (or boat) which is then screwed down onto a baseplate.  The baseplate has a hole in it for a cold probe to contact the boat from beneath.

The Invar baseplate is supported on three G-10 standoffs which provide thermal isolation and permit the ccd tilt to be adjusted.  The G-10 standoffs are screwed into the base of the dewar head.


SITe 2048 × 4096 CCD

MIT/LL 2048 × 4096 CCID-20

SITe boat + baseplate

LL boat + clamp piece

One side of the dewar head has a recessed sideplate (with o-ring) where we mount a preamplifier rigid-flex circuit board.  The component area of the pcb is rigid, and has a flex cable which solders to the 79-pin connector.  The internal board has two preamp circuits, filters for the clock and bias lines, and two temperature sensor circuits.


Hermetic 79-pin connector

Rigid-flex preamp board

The cold probe from the dewar cold surface contacts the ccd+boat from underneath.  A small temperature sensor and heater resistor are fitted onto the bottom of the boat to stabilize the temperature.


Dewar head with preamp and cooling strap

CCD installed in dewar head

Cold post and spring-loaded copper strap

Back o-ring surface


Test results -- Known Issues


Sample MIKE blue output -- OBJ CS2945-017 1800 sec binned 2x2 [.fits]


Sample MIKE red output -- OBJ CS2945-017 1800 sec binned 2x2 [.fits]

CCD Operation -- approx readout times and noise values
Mode Pixel time
Gain Noise
Readout (1×1)
Readout (2×2)
(µsec)
(e-/DN) ( e- )
(sec)
( sec )
Red (fast) --
1.0 4.6
90
30
Red (slow) --
1.0 3.5
160
48
Blue (fast) --
0.47 1.9
75
25
Blue (slow) --
0.47 1.8
140
42





Newly-completed MIKE goes from lab to telescope at sunset



Greg Burley (burley@ociw.edu)
Ian Thompson (ian@ociw.edu)