45 degree mirror to deflect the light 90 degrees, such that it points downwards for a horizontal target.
The cold mirror eliminates IR (thermal) light on the sample (Transmission > 85% for the region 800 - 1200nm, Reflection >90% for the region 425 - 650nm)

$ 989.00

This Sample Chamber will operate at either 77K or at room temperature, but does not include any mechanism to regulate the temperature between those points.
It requires a supply of liquid nitrogen in order to operate (sold separately).

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A custom temperature control system to allow operation at 77K or room temperature.

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A custom built sample chamber capable of both vacuum operation and a choice of temperature ranges between 77K and room temperature.
The system requires liquid nitrogen, but does not include it.

While the system will be constructed for this temperature range, the mechanisms, pumps, and other equipment is sold separately.
This Sample Chamber requires EITHER 188-8901 OR 188-8903 to complete the sample chamber. Please ask your authorized Sciencetech technical sales staff member for further information.

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A temperature control system to allow operation between 77K or room temperature.
This sisytem will come with two separate holders, each capable of holding a specific size and type of sample. They will not have the ability to rotate or moved, but will come prealigned for a fixed angle reflectivity, or transmission, through a motorized flipping mirror.

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Set of 6 optical density filters in values of 0.15, 0.3, 0.4, 0.6, 0.9, and 2.5. Each is 25 mm diameter and unmounted; the filter wheel is sold separately.
These are absorption filters and should not be used for high-powered applications (as opposed to reflective neutral density).

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The PTS-4-SSP is Sciencetech’s flagship measurement system. The PTS-4 includes all the extensive measurement tools and capabilities of the PTS-S/X and PTS-3-CPM and adds the powerful Steady State Photoconductivity (SSP) method. Steady state photoconductivity (SSP) measurements give information about the nature of defects, mobility-lifetime products, and the transport and recombination kinetics of photogenerated carriers. Since the states between quasi-Fermi levels act predominantly as recombination centres, steady state photoconductivity is sensitive to both the density and the nature of these states.

The PTS-4-SSP uses the PTS' integrated monochromatic light source to perform steady state photoconductivity measurements. To perform SSP measurements, the incident flux is first measured using the provided calibrated reference detector in AC mode. After system calibration is performed, the light source chopper is turned off and set to the open position for DC measurements.

Under DC illumination the photocurrent is measured at each wavelength using the included electrometer.

A relative value for the absorption coefficient can be obtained from studies of the sample using the included CPM technique.

Reflectivity measurements are not included with the system and are generally performed using a secondary instrument.

The volume generation rate can be calculated from the measured values of incident flux, the sample thickness, relative absorption coefficient and reflectivity profile. With measurements of the photocurrent and volume generation rate, the steady state photoconductivity can be determined.

Please speak to a Sciencetech Technical Specialist for further information.

PTS-4-SSP Includes:

-IV Testing
-Spectral Response
-Quantum Efficiency/IPCE
-CPM Measurements
-SSP Measurements

This system includes 4 IEC 60320 C13 compatible power cables. Region-specific version must be selected at the time of placing an order (see product 491-9001).

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The Sciencetech 9055 is a 250mm asymmetric focal length modified Czerny-Turner monochromator. It has a flat field output for use as a spectrograph. This model has an f/3.5 aperture (for the "Fast" version with f/2.5, please see the 9055F). It has a computer-controlled interchangeable turret for automatic grating and wavelength selection.
Both the input and output ports are located on the front faceplate of the monochromator, and the system includes one SS80 slit at the input port. CE compliant.

It Includes a Sci-Mono, a Windows based software module with a simple graphical user interface for controlling Sciencetech stepping monochromator wavelength selection. SciMono is provided free of charge with a Sciencetech motorized monochromator when SciSpec software has not been purchased. Sciencetech Software (Sci-Spec) is available at an additional cost. It is a standalone data acquisition and allows controlling the monochromator by itself. This system does not include gratings or a host computer. If you require any of these components, please speak with your technical sales staff member.

Refer to the technical datasheet for additional information.

This system includes 1 IEC 60320 C13 compatible power cables. Region-specific version must be selected at the time of placing an order (see product 491-9001).

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The PTS-3-CPM allows users the same ability to measure IV, Spectral Response, and Quantum Efficiency as the PTS-S or PTS-X, but adds the powerful Constant Photocurrent Method (CPM). The CPM system illuminates the sample solar sell with a bias solar light source while a separate light source is modulated to cover a specified spectrum. The bias source ensures that the signal is not dominated by the non-linear response at low-level illumination, but rather gives a baseline response dependent on the wavelength of the modulated source. This allows for a highly precise measurement of defect density. Please speak with a Sciencetech Technical Specialist for more information.
PTS-3-CPM Includes:
-IV Testing
-Spectral Response
-Quantum Efficiency/IPCE
-CPM Measurements

This system includes 3 IEC 60320 C13 compatible power cables. Region-specific version must be selected at the time of placing an order (see product 491-9001).
This system includes 1 IEC 60320 C5 compatible power cables. Region-specific version must be selected at the time of placing an order (see product 491-9002).

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The 9150 is Sciencetech's longest single path length monochromator with a 1.5 m focal length. Under optimum conditions with a 2400 l/mm grating it can achieve a resolution of 0.0065 nm in single pass mode. This model of monochromator accommodates a grating on a removable kinematic mount, allowing the user to manually swap one grating for another without losing alignment. Please note that this product includes one slit, but does not include any additional slits or a grating, these must be purchased separately. Please speak with a technical sales member for assistance in selecting the right components for your system. SciMono is included. For Sciencetech's full feature spectroscopy software, please see SciSpec (not included).

Please see the technical datasheet for additional information.

This system includes 1 IEC 60320 C13 compatible power cables. Region-specific version must be selected at the time of placing an order (see product 491-9001).

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Sciencetech's FSSP solar simulator is designed to illuminate targets of 1x1m with 1 sun, or smaller targets with multiple suns. The default spectral match is to ASTM AM1.5G. The flash itself is a stable 1ms length, with options available (purchased separately) to stretch the pulse. Timing and number of flashes can be computer controlled. This unit is a Class AAA flash solar simulator by default, with options available to reduce spatial uniformity in order to increase target size.

Sciencetech can also offer increased spectral ranges and other additional features upon request.

This product includes a flash system, power supply, lamp, and an air mass filter (AM1.5G). Other filters are available at additional cost. Available accessories include IV measurement systems, pre-configured host computers, and sample holding and cooling options. Please inquire with Sciencetech technical support staff about our automation and assembly line manufacturing partners.

Spectral Match: Class A
Spatial Non-Uniformity: Class A
Temporal Instability: Class A
Target Size: 1m × 1m (1 Sun) (Smaller targets available at higher intensities.)
Working Distance: 5-10m
Pulse Length: 1ms (Pulse stretching available)
Collimation: 2° half angle

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Sciencetech’s FSSP-HC-A highly collimated flash solar simulator is capable of illuminating targets up to 1.8 × 1.5m (or 1.5m diameter) with highly collimated light (up to 0.5° half angle). This allows testing of concentrated photovoltaics (CPV) or other applications requiring extremely high collimation. Within the illuminated area, the central 1 × 1m or larger meets Class A uniformity requirements. Please speak with your Sciencetech technical support staff for Class A uniformity matching over the entire illumination area. The default spectral match is to ASTM AM1.5D.

This product includes a flash system, power supply, collimating mirror, and lamp. Air mass filters are available separately (AM1.5D and AM1.5G, with additional filters available upon request). Available accessories include IV measurement systems, pre-configured host computers, and sample holding and cooling options. Please inquire with Sciencetech technical support staff about our automation and assembly line manufacturing partners.

Spectral Match: Class A
Spatial Non-Uniformity: Class A (Central 1m × 1m)
Temporal Instability: Class A
Target Size: 1.8m × 1.5m (1 Sun)
Working Distance: 5m
Pulse Length: 500µs at 90% of peak intensity, and 2.5ms at 50% of peak intensity
Collimation: 0.5° half angle

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Wavelength range: 250-800 nm
Dispersion: 8 nm/mm (When used with 9030 monochromator)

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This is a room-temperature detector for use with the SPS-300. This includes the DTGS detector with a mounting flange, but requires the use of a dual-phase lock-in amplifier (sold separately). Sciencetech's wideband detector design comes packaged in a mounting flange compatible with our SPS-300. It is connectorized to be powered directly from the Stanford SR-810/830 type lock-in amplifiers with a detachable cable. The spectral range is limited by window selection. This detector comes with a HDPE window standard.

Element size: 2.0 mm dia.
Spectral bandwidth: 16 to 100um (for HDPE window, other window materials available)
Frequency response: 10Hz - 265Hz (-3db points)
N.E.P.: 5x10-10 watts (@100Hz)
Power requirements: +/- 15 to +/- 24 volts max @ +/- 8 mA max.
Power connections:
DB-9M
Pins 2,3,4,5,9 no connection
+V In Pin 1
-V In Pin 6
Common Pin 7
Case GND Pin 8
Signal Connection: BNC

Suitable for direct connection to Stanford SR-810/830 lockin preamp power (not included).

This is a room-temperature detector for use with the SPS-300. This includes the DTGS detector with a mounting flange, but requires the use of a dual-phase lock-in amplifier (sold separately).

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This option includes all the components necessary to reach micro-Torr vacuum, including gauges, ports, valves, and both a roughing and turbo pump.
If only milli-Torr levels of vacuum are needed, please purchase the "SPS 300 Standard Vacuum Operation" upgrade instead.

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This includes all the necessary parts for vacuum operation including seals, valves, gauges, and port covers, as well as a roughing pump capable of reaching mTorr vacuum. The SPS-300 itself is capable of maintaining higher levels of vacuum operation, but requires a turbo pump in order to reach those levels of vacuum.
For higher vacuum operation (up to micro-Torr applications), please purchase the "SPS 300 Ultra-High Vacuum Operation" upgrade instead, as it includes all items listed here in addition to a turbo pump.

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The standard SPS-300 has a 50mm translating stage, wich can provide resolution up to 0.12 wavenumbers. The high resolution upgrade option extends the translating stage to 300mm, allowing the SPS-300 to achieve a resolution of 0.020 wavenumbers. Due to the increased stage length, an extension to the vacuum-sealed body is needed to accommodate the extra distance.

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This device is designed to be coupled to one of Sciencetech's IV Test systems. The Load Booster is inserted between the Keithley and the device under test with the Keithley current range set to 0.1A and used in remote (4 wire) sensing mode. The Load Booster effectively expands the IV testing current range.
Load Boosters may only be used in pulsed mode operation. They cannot be used for continuous illumination and measurement.
Voltage Range: 200V
Current Range: 10A

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Used to allow the SS150 to direct the beam downwards, upwards, or at 90 degrees to the usual output direction (horizontal). Not included in the Vertical Stand, due to the usual arrangement of allowing the beam to aim downwards (meaning in most cases this component is not required with the vertical stand option).

$ 655.00

This solar simulator is based on a Fresnel lens to collimate the light beam from the 3.0 kW Xe ozone-free arc lamp source, resulting in highly collimated illumination of the target spot. The spectral distribution of the xenon light source, along with the use of specially calibrated air mass filters, closely simulates the sun’s true spectral distribution in various conditions on Earth.

Works best with 1 Sun AM1.5G filters (included). Other AM filters are available but they may change the target size achievable. Contact a Sciencetech technical sales representative for details.

Target: up to 28 cm (11") diameter (depends on required irradiance level)
Collimation: 0.7° half angle (70% of irradiance is within)
Non-uniformity: Class B
Lamp: 3.0 kW ozone-free Xe short arc
Lamp Housing: air cooled
Illumination Direction: horizontal*
Power Supply: PS-XE3000-A-T

Includes: 30 cm (12") diameter UV transmitting Fresnel lens, intensity mask to produce class B (<5%) non-uniformity up to 11" diameter, igniter.

Power Requirements: 200-240 VAC, 50/60 Hz, 20 A. This system requires 1 NEMA 6-30P compatible power cables. Please select one region-specific power cable (see product 491-9004) at no cost.

Optional accessories: vertical beam turning unit, light intensity stabilizer, integrated motorized shutter
* Systems can be built for downfacing operation if specified at time of order

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