All rights reserved. No part of this publication may be reproduced by any means without the written
permission of Roper Scientific, Inc.
Printed in the United States of America.
SpectroPro is a registered trademark of Acton Research Corporation.
TAXI is a registered trademark of AMD Corporation
The information in this publication is believed to be accurate as of the publication release date. However,
Roper Scientific, Inc. does not assume any responsibility for any consequences including any damages
resulting from the use thereof. The information contained herein is subject to change without notice.
Revision of this publication may be issued to incorporate such change.
This manual provides the user with all the information needed to install a NTE/CCD
Detector and place it in operation. Topics covered include a detailed description of the
NTE Detector, installation, microscopy applications, cleaning, specifications and more.
Chapter 1
Detector.
Chapter 2, Detector Setup
installing it for spectroscopy or imaging, and over-exposure protection
considerations.
Chapter 3,
temperature control with a ST-133 or ST-138 Controller. Also provides
information on the effects of long-term vacuum degradation on cooling
capability and temperature control.
Chapter
and imaging applications.
Chapter 5, Microscopy Applications
Detector to a microscope. Includes discussion of various adapters, focusing
considerations and sensitivity to damage from EMF spikes generated by Xenon
or Hg arc lamps.
Chapter 6,
humidity, UV effects on the scintillator coating, baseline signal and noise.
Chapter 7,
optics.
Appendix A, Specifications
,
General Information
Cooling the Detector
4
, Focusing
Operation
Cleaning
discusses how to focus the detector in both spectroscopy
discusses a number of topics, including effects of high
contains directions for cleaning the detector’s housing and
provides an overview of the NTE/CCD
provides detailed directions connecting the detector,
discusses how to establish and maintain
discusses how to mount the NTE/CCD
includes detector specifications.
Appendix B, Outline Drawings
mount, C-mount, F-mount, and fiber-optic coupled detectors.
includes outline drawings of Spectrograph
Safety Related Symbols Used In This Manual
Caution! Risk of electric shock!
equipment indicates that one or more nearby items pose an electric
shock hazard and should be regarded as potentially dangerous. This
same symbol appears in the manual adjacent to the text that discusses
the hardware item(s) in question.
The use of this symbol on
8NTE/CCD Detector ManualVersion 2.A
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General Information
Chapter 1
Description
The NTE/CCD air-cooled detector or camera is ideally suited for medium light level
applications. State-of-the-art CCD arrays are available for the NTE/CCD that enable
outstanding performance in a wide range of applications for spectroscopy, biological
imaging, and physical science investigations.
Design
NTE/CCD detectors have three distinct sections. The front vacuum enclosure contains
the CCD array seated on a cold finger. This finger is in turn seated on a four-stage Peltier
thermoelectric cooler. The back enclosure contains the heat exchanger. An internal fan
cools the heat exchanger and the waste heat exits the unit through openings in the
detector housing.
The electronics enclosure contains the preamplifier and array driver board. This keeps all
signal leads to the preamplifier as short as possible, and also provides RF shielding.
Figure 1. NTE/CCD Detectors and Cameras
10NTE/CCD Detector ManualVersion 2.A
The NTE/CCD detector is available in both C-mount and F-mount configurations. See
Chapter 5 for detailed information on microscopy.
Detector Setup
This chapter covers the setup procedures for both imaging and spectroscopic
applications.
General Instructions
The following items are applicable to both imaging and spectroscopic systems.
Connecting the Detector
Each detector is supplied with a cable to connect to the controller. Make sure that the
controller is off, and then connect the larger end of the cable to the port marked
Detector
latch. The controller end of the cable, depending on the model of controller, is secured
by a slide-lock latch or by screws. Tighten the screws in place.
Controller Internal Switches
on the controller. The detector end of the cable is secured by a slide-lock
Chapter 2
Any user who will be running both NTE/CCDs
and
LN/CCDs with an ST-138 controller
must ensure that the internal power supply switches inside the controller are set properly.
Consult the controller manual for instructions on setting these switches. In the case of the
ST-133 Controller there are no internal switches.
If the system includes an ST-138 that was ordered with the NTE/CCD, the
Note:
internal switches will be properly set. These switches are only a consideration if an
already available controller is to be used with both NTE and LN detectors.
Gain Control
A gain control switch is provided on most
NTE/CCD detectors. This allows the user
to select one of three settings, LO, MED
and HI, which change the detector gain to
0.5×, 1× and 2×. This switch is active
when the detector is being controlled by an
ST-138. If an ST-133 controller is being
used, the switch is deactivated and gain
control is accessed in the software.
The gain of the detector should generally be
set so that the overall noise is ~1 count RMS.
In most instances this will occur w ith the
switch set to MED. If the array is a 1340 ×
100 or 1340 × 400 configured with the low-noise output, LO will probably be a more
WARNING: DO NOT OPERATE UNIT
WITHOUT PROTECTIVE COVERS.
CONTROLLER
GAIN
H
M
L
Figure 2. NTE Detector Rear Panel
Gain Control Switch
SHUTTER
12NTE/CCD Detector ManualVersion 2.A
suitable Gain setting. In situations where the A/D range exceeds that of the array, it will
generally be better to set the Gain to HI so that the signal can be spread over as much of
the A/D range as possible. This is a particularly important consideration in absorbance
measurements. Users who consistently measure low-level signals may wish to select HI,
which reduces some sources of noise. Users who measure high-level signals may wish to
select LO to allow digitization of larger signals. Customized values of gain can be
provided. Contact the factory for additional information.
Spectroscopy Se tup
This section describes how to set up the detector for spectroscopy applications.
Instructions for imaging applications appear later in this chapter. Microscopy
applications are discussed in Chapter 5.
Spectrograph Theory
In a typical spectrograph, light enters the
entrance slit and is collected by a
collimating mirror. Essentially, what a
spectrograph does is to form an image of
the entrance slit in the exit focal plane with
each position in the plane representing a
different wavelength. Collimated light
strikes the grating and is dispersed into
individual wavelengths (colors). Each
wavelength leaves the grating at a different
angle and is reimaged by a focusing mirror
onto a CCD detector at the exit focal plane.
As each wavelength images at a different
horizontal position, the spectrum of the
input light is spread across the CCD.
Individual wavelengths focused at different
horizontal positions along the exit port of
the spectrograph are detected
simultaneously. Rotating the diffraction
grating scans wavelengths across the CCD,
allowing the intensity at individual
wavelengths to be easily measured.
Focusing Mirror
Triple
Grating
Turret
CCD Port
CCD Focal Plane
Figure 3. Annotated Spectrograph Drawing
Collimating Mirror
Entrance
Slit
Array Orientation
For spectroscopy, the detector should be mounted so that the short axis of the CCD is
parallel to the entrance slit. The long axis will therefore correspond to the wavelength
axis of the spectrum. Because the NTE/CCD Detector is ordinarily not internally
shuttered in spectroscopy applications, the orientation of the CCD can be readily
determined by visual inspection of the faceplate. The faceplate cutout closely
corresponds to the dimensions of the underlying CCD array, which will itself be visible
through the window.
Chapter 2Detector Setup13
Square-format CCDs can also be used for spectroscopy, although they are more often
used in imaging applications. For square format CCDs (e.g. 512 × 512 or 1300 × 1340),
the user may orient the CCD to achieve binning along either direction of the CCD.
Binning along the rows (perpendicular mode) minimizes cross-talk and is therefore better
for multi-spectral applications. The drawback to this method is that scanning is slower
and noise may increase somewhat.
Binning along columns (parallel mode) provides maximum scan rate and lowest noise.
NTE/CCD users can easily switch between these orientations by simply rotating the
detector 90°.
Deep Focal Plane Spectrographs
Spectrographs with the focal plane
25 mm or more beyond the exit
interface are called deep focalplane spectrographs. Such
spectrographs include Acton
(adapters are available for all
Acton models), ISA HR320, ISA
HR640, Chromex 250IS, and most
instruments that are 1 meter or
longer. (If you are not sure of the
depth of the exit focal plane,
contact the spectrograph
manufacturer.)
Set screw
Flange 1
Figure 4. Adapter for a Deep Focal Plane Spectrogr aph
Flange 2Detector
Adapters for these spectrographs are generally in two pieces, as shown in Figure 4. The
generic assembly directions that follow can be used as a general guide.
Mounting Directions
1. Bolt Flange 2 to the NTE/CCD Detector using the screws provided.
2. Next, loosen the setscrews (3) on Flange 1.
3. Mount Flange 1 to the spectrograph.
4. Slide Flange 2 into Flange 1.
Do not tighten the setscrews until focusing and alignment are achieved as discussed in
Chapter 4.
Shallow Focal Plane
Shallow focal plane spectrographs are ones with a focal plane that is less than 25 mm
beyond the exit interface. The detector mount provided in these cases does not allow
focusing via the adapter. Focusing must be accomplished by adjusting the spectrograph.
The generic assembly directions that follow can be used as a general guide. However,
note that detailed instructions for your specific adapter are provided in the bag of adapter
parts.
14NTE/CCD Detector ManualVersion 2.A
Flange
Half-rings
Detector
Mounting Directions
1. Mount the flange to the detector using the
two half-rings and the screws provided.
Note that the tapered side of each half-ring
faces the adapter (Figure 5).
2. Next, thread the 10-32 hex screws
halfway into three of the six tapped holes
in the spectrograph’s exit plane.
3. Position the detector so the three hex head
screws line up with the openings in the
adapter flange.
4. Slide the detector over the screws and
rotate into the proper orientation.
5. Leave the detector free to rotate until it is
aligned as described in Chapter 4.
Figure 5. Shallow Focal Plane
Spectrograph Mounting Hardware
Entrance Slit Shutter
An entrance slit shutter can either be mounted on the entrance slit of the spectrograph or
used as a stand-alone shutter. Shutters for stand-alone operation have two tapped holes
for mounting to a stand: one metric, the other English.
Entrance slit shutter mounts come in two types. The first type (Figure 6) is for use with
CP-200 and HR-320 Spectrographs.
First Shutter Type Mounting Directi ons
1. Remove the Adapter Mount Cover by
removing the four Phillips head screws.
2. Place the Adapter Mount Body over the
entrance slit.
3. Mount it by threading the Retainer to the
spectrograph.
4. Replace the shutter and the Adapter
Mount Cover.
Adapter Mount Cover
Spectrometer
Adapter Mount Body
Retainer
Figure 6. One Type of Entrance Slit
Shutter Mount
Chapter 2Detector Setup15
Second Shutter Type Mounting Directions
The second shutter mount, used with all Acton Research
Spectrometer
Adapter
spectrographs, requires no disassembly. Mount it to the
spectrograph as shown in Figure 7.
Figure 7. Entrance Slit Shutter for
Acton Spectrographs
The shutter cable should be connected to the Shutter Power connector on the rear panel
of the NTE/CCD Detector or to the Shutter Power connector on the ST-133 Controller.
In many systems, cable length considerations will make it more convenient to connect to
the Shutter Power connector on the detector.
WARNING
:
Dangerous live potentials are present at the Remote
Shutter
power
connector. To avoid shock hazard, the Controller power should be OFF when connecting
or disconnecting a remote shutter.
Overexposure Protection
Imaging
Detectors that are exposed to room light or other continuous light sources will quickly
become saturated. This most often occurs when operating without a shutter. Saturation is
not harmful to a non-intensified detector. To reduce the incident light, close the entrance
slit of the spectrograph completely.
This section describes how to connect lenses to the detector for imaging applications.
Instructions for spectroscopic applications appear later in this chapter. Microscopy
applications are discussed in Chapter 5.
NTE/CCD Detectors use either a C-mount or a Nikon bayonet adapter. If you cannot use
the adapter you received, contact the factory for technical support or replacement. See
page 50 for Information on accessing the Roper Scientific Technical Support Dept.
Nikon (F-mount) Bayonet
To attach an F-mount lens to the detector, the unit must be equipped with an F-mount
adapter. The adapter type must be specified at the time of purchase.
16NTE/CCD Detector ManualVersion 2.A
To Mount the Lens on the Detector:
Set screws to lock front
1. Locate the large indicator dot on the side of the
part of adapter in place
lens.
2. Note the corresponding dot on the front side of the
adapter.
3. Line up the dots and slide the lens into the
adapter.
4. Turn the lens counterclockwise until a click is
audible. The lens is now locked in place.
Lens release lever
Front part of adapter
for adjusting focus
5. In addition to the focusing ring of the lens, there is
provision for focusing the adapter itself. The
Figure 8. Nikon Lens Adapter
adjustment is secured by #4-40 setscrews on the
inside of the adapter. Directions for focusing the
lens and the adapter are provided in Chapter 4.
To Remove the Lens:
1. Locate the lens release lever at the front of the lens mount.
2. Press the lever toward the detector housing and simultaneously rotate the lens
clockwise.
3. Then pull the lens straight out.
Although microscopes more commonly are used with a C-mount adapter, operation with
a detector having an F-mount adapter may also be possible. See Chapter 5, MicroscopyApplications and the adapter literature for further directions.
C-mount
NTE/CCD detectors can be ordered with an integral C-mount adapter. C-mount lenses
simply screw into the front of these detectors. Tighten the lens by hand only. See Chapter
5 for information on connecting to a microscope.
C-mount detectors are shipped with a dust cover lens installed. Although this lens
Note:
is capable of providing surprisingly good images, its throughput is low and the image
quality is not as good as can be obtained with a high-quality detector lens. Users should
replace the dust-cover lens with their own high-quality laboratory lens before making
measurements.
Overexposure Protection
Set the lens to the smallest aperture (highest F-number) and cover the lens with a lens
cap to prevent overexposure.
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