Nireos Hera Iperspettrale SWIR

Spectral range = 900 – 1700 nm
Sensor spatial resolution = 640 x 512 pixels
User adjustable spectral resolution: < 5 nm @ 900 nm/ <20 nm @ 1700 nm Sensor = cooled InGaAs (?T = 30?) Number of bits = 14 bits Software interface = Labview based interface Number of spectral bands = ?* Field of view = 11 degrees Working distance = 1 m - ? Dimensions = 220 x 160 x 105 mm Weight = 2.85 kg * HERA is FT spectroscopy based instrument and number of spectral bands is software selectable and independent from measurement time

SKU: Nireos Hera Iperspettrale SWIR Category: SWIR Tag: Mounted

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HERA IPERSPETTRALE is a compact and rugged camera that enables an innovative approach to spectral imaging.
With its unique and patented technology based on time-domain Fourier Transform (FT) detection, HERA provides exceptional spatial-spectral resolution and superior sensitivity in low-light illumination conditions.
HERA is based on a Fourier Transform (FT) approach: the data-cube is acquired in the time-domain, by step-scanning a compact ultra-stable interferometer in front of the bidimensional sensor.
The software then automatically computes an FT at each and every pixel of the image, providing the final hyperspectral data-cube.
As a result of an FT, the spectrum at each pixel is a continuous curve, so the number of bands is virtually unlimited, not defined by the hardware.
As in any other FT techniques, the spectral resolution is not constant as a function of the wavelength. Also, the spectral resolution can be simply varied via software: at each measurement, you can decide whether to acquire a high spectral resolution-image, or – if not required – a faster and lower spectral resolution-image.
Regardless of this choice, the exceptional light throughput is not affected, thanks to the FT approach.

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	Nireos Hera Iperspettrale SWIR remove	Specim Fenix remove	HySpex VNIR-1800 remove	Resonon Pika IR-L remove	Specim FX17 remove	Specim FX50 remove
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Content	HERA IPERSPETTRALE is a compact and rugged camera that enables an innovative approach to spectral imaging. With its unique and patented technology based on time-domain Fourier Transform (FT) detection, HERA provides exceptional spatial-spectral resolution and superior sensitivity in low-light illumination conditions. HERA is based on a Fourier Transform (FT) approach: the data-cube is acquired in the time-domain, by step-scanning a compact ultra-stable interferometer in front of the bidimensional sensor. The software then automatically computes an FT at each and every pixel of the image, providing the final hyperspectral data-cube. As a result of an FT, the spectrum at each pixel is a continuous curve, so the number of bands is virtually unlimited, not defined by the hardware. As in any other FT techniques, the spectral resolution is not constant as a function of the wavelength. Also, the spectral resolution can be simply varied via software: at each measurement, you can decide whether to acquire a high spectral resolution-image, or - if not required - a faster and lower spectral resolution-image. Regardless of this choice, the exceptional light throughput is not affected, thanks to the FT approach.	Fenix FENIX is optimized for the most demanding geological, law enforcement, and environmental applications. In a single continuous image, FENIX spectral camera delivers the best hyperspectral data ever seen over VNIR, NIR, and SWIR wavelengths. FENIX offers extreme ruggedness and 75% reduction in size and weight compared to previous multi-sensor systems. The excellence in technical performance and physical size has been achieved through innovative and unique ?single optics dual spectrograph? design.	HySpex VNIR-1800 The HySpex VNIR-1800 hyperspectral camera is developed for field, laboratory, and airborne applications. HySpex VNIR-1800 utilizes a cutting edge actively cooled and stabilized scientific CMOS detector. This makes VNIR-1800 the ideal camera for high-end data acquisitions where high radiometric accuracy is required. The dynamic range of 20 000 ensures outstanding SNR levels even in darker areas of an image of highly dynamic scenes. With a max frame rate of 260 fps, combined with aberration-corrected optics and high optical throughput (f/2.5), HySpex VNIR-1800 offers a unique combination of data quality, high speed, and sensitivity. A wide range of close-up lenses allows the use of the camera at working distances ranging from a few centimeters with a spatial resolution of 24 ?m to infinity e.g. airborne remote sensing.	Pika IR-L 925 - 1700 nm Lightweight Infrared The Pika IR-L is a lightweight and compact Near-Infrared (925-1,700 nm) imager. The small size and mass make it well suited for airborne applications, where it can provide invisible to the naked-eye contrast of outdoor features. For a compact, lightweight Visible light spectral range option, please see the Pika L. For a higher spectral and spatial resolution version of the Pika IR-L, please see the Pika IR-L+ imager.	Specim FX17 Specim FX17 hyperspectral camera operates in the near-infrared region and can literally see the invisible. It can reveal the targets? chemical composition, moisture, and foreign objects that are invisible to the human eye. Specim FX17 can, for example, detect different plastic types for recycling and measure the sugar level of fruits and vegetables and the moisture percentage of baked goods.	Specim FX50 Specim FX50 is the only hyperspectral camera on the market covering the full mid-wave infrared (MWIR) spectral range of 2.7 - 5.3 ?m required, for example, in black plastics sorting. Specim FX50 is a high-speed, accurate, and efficient line-scan hyperspectral camera designed specifically for industrial environments.
Description	Spectral range = 900 - 1700 nm Sensor spatial resolution = 640 x 512 pixels User adjustable spectral resolution: < 5 nm @ 900 nm/ <20 nm @ 1700 nm Sensor = cooled InGaAs (?T = 30?) Number of bits = 14 bits Software interface = Labview based interface Number of spectral bands = ?* Field of view = 11 degrees Working distance = 1 m - ? Dimensions = 220 x 160 x 105 mm Weight = 2.85 kg * HERA is FT spectroscopy based instrument and number of spectral bands is software selectable and independent from measurement time		Spectral range = 400 - 1000 nm Spatial pixels = 1800 Spectral channels = 186 Spectral sampling = 3.26 nm FOV* = 17? Pixel FOV across/along* = 0.16/0.32 mrad Bit resolution = 16 bit Noise floor = 2.4 e- Dynamic range = 20000 Peak SNR (at full resolution) > 255 Max speed (at full resolution) = 260 fps Power consumption = 30 W Dimensions (l-w-h) = 39 - 9.9 - 15 cm Weight = 5.0 kg Camera Interface = CameraLink *Can be doubled with FOV expander	Spectral Range (nm) = 925 - 1700 Spectral Channels = 236 Spectral Bandwidth (nm) = 3.3 Spectral Resolution - FWHM (nm) = 5.9 Spatial Pixels = 320 Max Frame Rate (fps) = 364 f/# = 1.8 Interface = GigE Dimensions (mm) = 210 x 68 x 63 Weight, w/o lens (kg) = 1.01	Spectral Range = 900-1700 nm Spectral resolution (FWHM) = 8 nm (mean) Spectral sampling/pixel = 3.5 nm Spectral bands = 224 With default binning Numerical aperture = 1.7 With default lens Optics magnification = 0.80 Effective pixel size = 18.7 ?m At fore lens image plane Effective slit width Physical width = 42?m. Projection on sensor = 32 ?m (M=1.3) At fore lens image plane Effective slit length = 12.0 mm At fore lens image plane SNR @ max. signal = 1000:1 Bit depth = 12 Maximum frame rate = 670 (FX17)/ 527 (FX17e) FPS full range Binning = 1,2,4 spectral and spatial Default: 1 spectral x 1 spatial ROI = Freely selectable multiple bands of interest. Minimum height of ROI is two 1-binned rows. Maximum frame rate is determined by total number of rows between first row of first mROI and last row of last mROI and the total number of rows included in the mMROI?s. Pixel operability = 99.5%. Allowed clusters: Size 2-6 pixels: N/A/ Size 7-12 pixels: ? 6/ Size 13-19 pixels: ? 2/ Size 20-35 pixels: ? 1/ Size > 35: 0 Image corrections = Non uniformity correction/ Bad pixel replacement/ Automatic Image Enhancement (AIE)/One point NUC. AIE: Unified spectral calibration + corrected smile and keystone aberrations Sensor material = InGaAs Sensor cooling = TEC Full well capacity = 1.44 Me- Read-out modes = IWR / ITR Optics temperature = Passive Default is 20 degrees Celsius Lens mount = Custom mount Fore lens FOV options = 12 deg/38 deg (default)/53 deg/66 deg/75 deg/90 deg. Only the default lens is specifically designed for FX17. With other lens options, optical parameters may vary. Camera digital data output/control interface = GigE Vision, CameraLink Camera control protocols = GenICam, ASCII Power input = 12 V DC (+-10%) Power consumption = Max 24 W Connectors = Industrial Ethernet OR CameraLink (standard MDR 26-pin). Power - Fischer 12pin DBPLU1031Z012\|130G IP = IP52 Dimensions (L x W x H) = 150 x 75 x 85 mm Mounting surface option on three sides. Mounting kit adds 24 mm distance on mounting side. Weight = 1.56 kg Storage temperature = -20 ... +50 oC (non-condensing) Operating temperature = +5 ... +40 oC (non-condensing) Relative humidity = 5% - 95% (non-condensing)	Spectral Range = 2.7 - 5.3 ?m Spectral resolution (FWHM) = 35 nm Spectral sampling/pixel = 8.44 nm, Without binning Spectral bands = 154, With default binning Numerical aperture = 2.0 Optics magnification = 0.5 Effective pixel size = 30 ?m, At fore lens image plane Effective slit width = 104 ?m, At fore lens image plane Effective slit length = 19.2 mm, At fore lens image plane Dynamic Range = 1600:1 with 1.5 ms exposure time Usable dynamic range / noise Spatial samples = 640 Bit depth = 16 Maximum frame rate = 380 fps, Full image with default binning Binning = 1,2,4 spectral and spatial, Default: 2 spectral x 1 spatial ROI = Freely selectable multiple bands of interest. Minimum height of ROI is two 1-binned rows. Maximum frame rate is determined by total number of rows between first row of first mROI and last row of last mROI - not the total number of rows included in the mMROI?s. Pixel operability = Number of operable pixels >99.7%. Allowed clusters: Size 4-8 pixels: <= 12/ Size 9-12 pixels: 2/ Size 13-19 pixels: 1/ Size >19 pixels: 0 Image corrections = Non uniformity correction/Bad pixel replacement/Automatic Image Enhancement (AIE). One point NUC. AIE: Unified spectral calibration + corrected smile and keystone aberrations Sensor material = InSb Integrated cooler = Stirling Up to 10000 hours Full well capacity = 5.1 Me- Read-out modes = IWR / ITR Optics temperature = TEC-stabilized Default is 20 degrees Celsius Lens mount = Custom mount Fore lens options = OLEM43, OLEM23, OLEM17 Field of view = 24 deg, 45 deg, 60 deg Camera digital data output/control interface = GigE Vision, Custom ethernet Camera control protocols = GenICam, JSON-RPC Power input = 24 V DC Power consumption = Max 90 W, Typical 40 W, During simultaneous cool-down of optics and detector Connectors = Ethernet/ Aux - 0306423 (09-0428-90-08) Binder 8pin/ Power - 0306627 (LF10WBR-4P) Hirose 4pin Trigger in IP = IP40 Dimensions (L x W x H) = 280 x 202 x 169 mm Mounting surface option on three sides. Mounting kit adds 24 mm distance on mounting side. Weight = 7 kg Storage temperature = -20 ... +50 oC Operating temperature = +5 ... +40 oC Relative humidity = 5% - 95% (non-condensing)