Sciencetech's (SCP-SP-T) is a micropositioning probe station with a magnetic base and a tungsten needle-tip probe. It utilizes thumbscrews for adjustment. 0.3” is the magnitude of fine adjustment for this probe.

Tungsten needle-tip probes are an excellent choice for applications requiring highly accurate, fine probe placement.

$ 1,150.00

This vertical stand enables the SS150 fully reflective solar simulator to project its output beam downwards onto a horizontal illumination table which makes it ideal for solar cell testing.

$ 1,160.00

Adjustable CCD mount for 124-9045, (CCD-S3600-D-UV) Advanced Digital CCD Line Camera. This mount is compatible with all Sciencetech standard and high-resolution monochromators.

$ 1,211.00

An arc lamp is not designed to be frequently turned off and on and doing so will dramatically lower its service life. In addition, each time it is turned on it requires the power supply to ignite it with a 20,000V+ spark. THe best option for performing exposure testing is to integrate an electronic shutter system inside the beam homogenizer. The electronic shutter is computer controlled with an activation time of <150ms. Software for the shutter controller is included with this item. The standard shutter controller connects to a computer via RS232. RS232-USB converters are available and work with this product. In addition to computer control the shutter can be controlled via a toggle switch on the shutter controller box.

This shutter can be used with any high powered light source and can effectivley block a 5" diameter beam. See the brochure information for a mounting pattern.

This device can be controllable through Sciencetech's new line of Touch Screen power supplies (including automated explosure time control).
Please note leaving the shutter closed for exteremly long periods of time while the arc lamp is on may cause damage to the motorized components.

$ 1,308.00

Sciencetech’s (SCP-SP-G) is a micropositioning probe station with a magnetic base and a gold-plated spring probe. It utilizes thumbscrews for adjustment. 0.3” is the magnitude of fine adjustment for this probe.

Gold spring probes are an excellent choice for most applications, with the probe tip gently contacting the surface of your test device. For applications requiring finer probe placement, please see our tungsten needle-tip probe stations.

$ 1,312.00

Multialkali high sensitivity side-on PMT
Spectral range: 185-900 nm,
Peak sensitivity wavelength: 400nm
Glass UV Envelope

Photocathode Area Size 8 x 24 mm
Photocathode Material Multialkali
Window Material UV glass
Dynode Structure Circular-cage
Anode to Cathode Voltage 1250 V
Average Anode Current 0.1 mA
Anode to Cathode Supply Voltage 1000 V
Luminous Sensitivity Min. 140 μA/lm
Luminous Sensitivity Typ. 250 μA/lm
Radiant Sensitivity Typ. 74 mA/W
Anode Luminous Sensitivity Min. 400 A/lm
Anode Luminous Sensitivity Typ. 2500 A/lm
Anode Radiant Sensitivity Typ. 7.4e5 A/W
Anode Dark Current (after 30min.) Typ. 3 nA
Anode Dark Current (after 30min.) Max. 50 nA
Time Response Rise Time Typ. 2.2 ns
Time Response Transit Time Typ. 22 ns

$ 1,312.00

A 300W xenon short arc lamp bulb, using a fused silica glass envelope. Please note that this lamp produces ozone.

$ 1,364.00

The CTBT-RF is designed to work with Sciencetech's line of SS solar simulators (between 500W and 1.6kW). The CTBT-RF is designed to hold 3" x 4" cold mirrors. A heat sink is mounted behind the dichroic turning mirror to capture transmitted light. The CTBT-RF turns the beam 90 degrees from the standard horizontal output.


Four different cold mirror options exist (purchased separately):
1) 275-375nm
2) 325-450nm
3) 350-550nm
4) 450-725nm
5) UV Enhanced aluminum mirror (250-3000nm)


Please speak with your Sciencetech representative for ordering information.

$ 1,364.00

This Broadband Thermopile Detector allows the measurement of total broadband radiation emitted by a light source. It could also be used to measure the light power density on a surface (in W/cm2) which is particularly useful for uniformity measurements and for checking solar simulator performance. This detector has a 19mm diameter sensor and picks up all wavelengths between 190-11μm (UV-VIS-IR). Please note that this detector head requires either an external display controller or computer interface (sold separately) to show the measured power. The price shown includes the detector head, post, post holder, and base only. (1mW NEP).

This thermopile is recommended for high-powered light sources (such as focused 500W + arc lamps) and concetrator solar simulators (5 Suns +, 500 mW/cm2).

$ 1,389.00

An AM0 filter compatible with Sciencetech solar simulators, including FT-style filter holder. Filter clear aperture is a diameter of 76 mm (3"). Please select the product line the filter is intended to be used with to ensure the proper spectral output.

AM0 simulates the solar spectrum just outside Earth’s atmosphere, where there is very little atmosphere-related absorption of solar radiation. This is generally used for space applications.

$ 1,394.00

An AM1.5D filter compatible with Sciencetech solar simulators, including FT-style filter holder. Filter clear aperture is a diameter of 76 mm (3"). Please select the product line the filter is intended to be used with to ensure the proper spectral output.

AM1.5D simulates the terrestrial solar spectrum on the ground when the sun is at a zenith angle of 48.2°. It includes only direct light from the sun, and not the diffuse light that is scattered by the atmosphere. As a result, this filter simulates the direct radiation which reaches the ground.

Please note that for some simulator models the same filter is used to supply an AM1.5G spectral match. Purchasing separate AM1.5G and AM1.5D filters for the same model simulator may not provide a different spectrum.

$ 1,394.00

An AM1.5G filter compatible with Sciencetech solar simulators, including FT-style filter holder. Filter clear aperture is a diameter of 76 mm (3"). Please select the product line the filter is intended to be used with to ensure the proper spectral output.

If the filter is not intended to be used with a Sciencetech solar simulator, the product line "None" may be selected, but the spectral output cannot be guaranteed when paired with a non-Sciencetech source.

AM1.5G simulates the terrestrial solar spectrum on the ground when the sun is at a zenith angle of 48.2°. It includes both direct light from the sun, and the diffuse light that is scattered by the atmosphere. As a result, this filter simulates the total radiation, known as global radiation, which reaches the ground.

$ 1,394.00

This data acquisition module features 3 analog inputs via BNC connectors. The data acquisition board is 16-bit and can measure a single channel up to 50 kS/s. An additional BNC connector for a multi-purpose digital input/output can be used to time measurements and/or send signals to external hardware such as a high speed shutter.

This module includes 1 BNC cable and 1 USB cable so that it is ready to interface with a single channel detector such as a PMT or Si photodiode detector (sold separately). For spectroscopy systems the SciSpec Windows application software to interface with a Windows Based PC is required and is sold separately.

Multi-channel data acquisition is possible using SciSpec software, if this option is required please speak to a Sciencetech technical sales representative.

$ 1,413.00

A Beam Turning Assembly can be mounted to the output port of many of Sciencetech's Solar Simulators to redirect the light downwards onto a sample platform. The Beam Turner may also be used to adjust the light path to any 90° angle perpendicular to the horizontal output beam.

$ 1,414.00

This Broadband Thermopile Detector allows the measurement of total broadband radiation emitted by a light source. It could also be used to measure the light power density on a surface (in W/cm2) which is particularly useful for uniformity measurements and for checking solar simulator performance. This detector has a 19mm diameter sensor and picks up all wavelengths between 190-11μm (UV-VIS-IR). Please note that this detector head requires either an external display controller or computer interface (sold separately - see below) to show the measured power. The price shown includes the detector head, post, post holder, and base only.

This thermopile is recommended for high-powered light sources (such as focused 500W + arc lamps) and concetrator solar simulators (5 Suns +, 500 mW/cm2).

$ 1,432.00

Wavelength range: 300-1200 nm
Dispersion: 12 nm/mm (When used with 9030 monochromator)

$ 1,465.00

Wavelength range: 800-3200 nm
Dispersion: 32 nm/mm (When used with 9030 monochromator)

$ 1,510.00

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

$ 1,510.00

This is an upgrade to Sciencetech's line of high resolution monochromators, including the 9040, 9490, 9150, and the double pass versions of these monochromators. This allows the use of two output ports on the system. It also includes a manual flipping mirror to select between the two ports. It does not include a second slit, any coupling optics for sample chambers, or coupling mechanisms for CCDs. These must be purchased separately.

Mirror UV Enhanced Aluminum
Coating Ravg >85% @190-2000nm

Contact for Pricing

This is an upgrade to Sciencetech's line of high resolution monochromators, including the 9040, 9490, 9150, and the double pass versions of these monochromators. The upgrade includes both the port itself and a manual flipping mirror to allow selection of input port. It does not include another slit, any coupling optics for sample chambers, or coupling mechanisms for CCDs. These must be purchased separately.

Mirror coating
UV Enhanced Aluminum
Coating Ravg >85% @190-2000nm

Contact for Pricing