Maury MW - Cryogenic Noise Standards - NBS Series
- Expandable frequency range from 18 to 325 GHz
- 2 to 3 times better accuracy
- Automatic Nitrogen purge eliminates helium equipment
- Primary calibration standard
- Radiometer reference source
- SATCOM earth station conformance verifications
The NBS-Series consists of calibration standards based on the primary fundamental physic constants of thermal noise and blackbody radiation. This provides the ultimate accuracy when measuring extremely low noise figures (noise temperatures). Simple, and versatile to use, the NBS-Series is an ideal solution for noise source calibrations, radiometer test references and low noise amplifier tests.
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Frequency Range |
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Expandable frequency range from 18 to 325 GHz |
More Product Information
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Defect pixel correction (on/off)
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Fixed pattern noise correction (on/off)
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Region of interest (ROI)
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Gain (manual control, 0 to 20 dB)
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Exposure (manual control, 44.2 µs to 1.4 s)
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Gamma correction
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Reverse X
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DeviceLinkThroughputLimit (easy bandwidth control)
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Sync out modes: Waiting for a trigger, exposing, readout, imaging
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Storable user sets
Not all amplifiers are created equal, so how can you be certain that an amplifier will work for your needs? You deserve to be confident that the amplifiers used with your test-and measurement lab benches will meet the requirements of your specific applications, are reliable, and are equally well-supported pre-and post-sale. When it comes to application expertise, reliability and support, there is no company that does it better than Maury.
Flexibility
- Different substrate carriers for wafers up to 200 mm or single dies
- Probe cards and/or up to eight positioners
- Use with liquid nitrogen or helium, depending on the target temperature. Or use of cryo-cooler for dry-cooling option.
- Accessories available, such as black bodies and optical motion analysis tools
- Optional upgrade for 300 mm wafer
- Designed for industrial environments
- Covers wide range of measurements (I-V, C-V, RF, MEMS, OPTO)
- Ideal for small structures
See "Specifications & Details" tab for more key features
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Auto gain (manual gain control: 0 to 22 dB)
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Auto exposure (manual exposure control: 100 µs to 1 s, 1 µs increments)
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Binning (horizontal and vertical) (sum)
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Decimation X/Y
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Enhanced Defect Pixel Correction (DPC)
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Fixed Pattern Noise Correction (FPNC)
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Gamma correction
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Three look-up tables (LUTs)
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Region of interest (ROI)
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EF lens control (order option -18)
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Event channel
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Image chunk data
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IEEE 1588 Precision Time Protocol (PTP)
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RS232
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Storable user sets
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StreamBytesPerSecond (bandwidth control)
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Stream hold
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Sync out modes: Trigger ready, input, exposing, readout, imaging, strobe, GPO
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Temperature monitoring (main board and sensor board)
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Trigger over Ethernet (ToE) Action Commands
- High ENR
- Wide frequency range
- Custom frequencies available
The NC3600 Series coaxial noise sources are an excellent choice for applications requiring high ENR, such as ATE, radiometer, and radar systems.
An SMA male connector is standard for the RF output and feed thrus for bias input. SMA female is an option. Custom frequencies and flatness available. Contact the factory with your request.
- 5” touch screen display
- Noise output through female N connector
- Ethernet connection for remote control
The NGX1000 programmable noise generator is a high performance, broadband additive white gaussian noise (AWGN) generator in an easy-to-use compact form factor. The streamlined user interface and flat menu structure provides a fast, simple way to add RF noise in a communications system to test reliability, robustness and performance.
All functionality of the generator is accessible through the 5” touch screen or via remote control through an ethernet connection delivering flexible, programmable noise generation for broad use in semiconductor, military, aerospace, satellite, medical and communications applications.
- Ideal probe for up to 48 V power conversion
- 250, 500 MHz and 1 GHz bandwidth
- 80 V dynamic range
- 60 V common mode
- Highest accuracy
- 0.5% gain accuracy
- Precision gain calibration
- Best LF flatness (0.1 dB)
- Lowest noise and highest rejection
- Wide variety of tips
- High performance solder-in
- Browser
- Single pins and header
- Mini and micro grabbers
- Socketed connections
- High temp solder-in
- Y-banana adaptor
- ProBus active probe interface
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Defect pixel correction (on/off)
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Fixed pattern noise correction (on/off)
-
Region of interest (ROI)
-
Gain (manual control, 0 to 20 dB)
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Exposure (manual control, 44.2 µs to 1.4 s)
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Gamma correction
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Reverse X
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DeviceLinkThroughputLimit (easy bandwidth control)
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Sync out modes: Waiting for a trigger, exposing, readout, imaging
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Storable user sets
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High SNR mode (up to 24 dB better signal-to-noise ratio)
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Low-noise binning mode
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Shading correction
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Defect pixel correction
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Area of interest (AOI), separate AOI for auto features
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Binning
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Decimation
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Auto gain (manual gain control: 0 to 24.4 dB)
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Auto exposure (39 µs to 67 s)
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Auto white balance
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Look-up table (LUT)
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Hue, saturation
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Color correction
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Local color anti-aliasing
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Reverse X/Y
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Deferred image transport
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Trigger programmable, level, single, bulk, programmable delay
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Sequence mode (changes the camera settings on the fly)
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SIS (secure image signature, time stamp for trigger, frame count etc.)
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Storable user sets
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Camera and IEEE 1394b cable (other configurations on request)
Maury Microwave
Maury Microwave is a pioneering leader in the design and manufacture of precision RF and Microwave calibration, test & measurement, and modeling solutions that are powering global efforts toward a more secure, more connected, future.
Maury Microwave offers Measurement and Modeling Device Characterization Systems and Services including nonlinear passive, active and hybrid-active fundamental and harmonic load pull, non-50Ω X-Parameter modeling, pulsed IV Pulsed s-parameters and compact transistor modeling, and patent-pending ultra-fast/accurate noise parameters.