NIRvana: 640ST. Applications: Nanotube fluorescence, emission, absorption, non-destructive testing and singlet oxygen detection

Similar documents
Easy integration into complex experimental setup

NIRvana: 640. Applications: Nanotube fluorescence, emission, absorption, non-destructive testing and singlet oxygen detection

20 MHz/16-bit readout 61 fps rate at full-frame resolution. Use ROI/binning for hundreds of frames per second.

ProEM -HS:1024BX3 FEATURES BENEFITS

PIXIS-XO: 400B 1340 x 400 imaging array 20 x 20 µm pixels

PyLoN: Applications: Astronomy, Chemiluminescence, Bioluminescence, Phosphor Imaging, Ultra-low light Imaging and Spectroscopy.

PI-MAX 4: 1024 x 256 SPECTROSCOPY GROUP

Applications: Astronomy, Photometry, EL/PL Imaging, Luminescence & Fluorescence Imaging, and Bose-Einstein Condensate (BEC) Page 1 of 7 IMAGING GROUP

Quad-RO: 4320 X-RAY GROUP

ProEM -HS:1KBX3-10µm

ProEM -HS:1024BX3 FEATURES BENEFITS

IMAGING GROUP. 512 x 512 imaging array; 24 mm x 24 mm pixels Scientific grade CCD All-metal, hermetic vacuum seals; Lifetime vacuum guarantee

Minimizes reflection losses from UV - IR; Optional AR coatings & wedge windows are available.

IMAGING GROUP x 1300 imaging array; 20mm x 20mm pixels Scientific grade CCD All-metal, hermetic vacuum seals; Lifetime vacuum guarantee

PIXIS: 512 IMAGING GROUP

IMAGING GROUP x 2048 imaging array; 13.5mm x 13.5mm pixels Scientific grade CCD All-metal, hermetic vacuum seals; Lifetime vacuum guarantee

Compatible with Windows 8/7/XP, and Linux; Universal programming interfaces for easy custom programming.

PI-MAX 4: 1024 x 256

Back-illuminated scientific CMOS cameras. Datasheet

PI-MAX 4: 1024 EMB. Applications:

PI-MAX 4: 1024i-RF. Compatible with Windows 8/7/XP, and Linux; Universal programming interfaces for easy custom programming.

Video frame rates and higher to efficiently synchronize with high repetition rate lasers

FEATURES BENEFITS 1024 x 1024 Imaging Array High resolution imaging and spectroscopy

SOPHIA 2048B. Datasheet ULTRA-LOW-LIGHT, LOW-NOISE UV / VIS CAMERAS LARGE-FORMAT CCD CAMERAS

PI-MTE3. Datasheet LARGE-FORMAT, IN-VACUUM CAMERAS. Direct detection of soft x-rays. Up to 4k x 4k sensor formats. Reads out as fast as 3 full fps

pco.1600 cooled digital 14 bit CCD camera system

pco.1600 cooled digital 14 bit CCD camera system

SOPHIA -XO 2048B SOPHIA -XO 4096B

. Ideal for fast, shutterless imaging

SYNCERITY TM 1024 x 256

DV887 (back illuminated)

Revolutionary High-Speed Cameras for Spectroscopy

Frequently Asked Questions: Princeton Instruments excelon TM CCD and EMCCD Cameras

sensicam qe cooled digital 12bit CCD camera system

Frequently Asked Questions: excelon Back Illuminated CCD/EMCCD Cameras

25.6 mm wide / 1600 pixel, 3 MHz Spectroscopy EMCCD. Specifications Summary 1. Output node well depth: Conventional mode Electron Multiplying mode

Specifications Summary 1. Array Size (pixels) Pixel Size. Sensor Size. Dark Current 2. Pixel Well Depth (typical) e e -

Newton EMCCD. Specifications Summary 1. Output node well depth (typical) High Sensitivity mode Electron Multiplying mode

Product Information Version 1.0. ZEISS Axiocam 506 mono Your High Resolution Microscope Camera for Live Cell Imaging Fast, Flexible, and Sensitive

Lt Megapixel High-Speed CMOS Camera with SuperSpeed USB 3.0

ikon-xl 230 VERY LARGE AREA ASTRONOMY CCD P P P CCD NEW

High resolution Low noise High dynamic range Unparalleled sensitivity. Vision At Its Best

idus 401 Series Specifications Summary Active pixels 1024 x 127 Register well depth (typical) 1,000,000 e - Maximum spectra per sec 88

800 nm µm Spectroscopy InGaAs PDA. Specifications Summary. Active pixels 512 or Pixel well depth (typical)

Product Information Version 1.1. ZEISS Axiocam 503 mono Your Flexible and Sensitive 3 Megapixel Microscope Camera for Live Cell Imaging

Confocal Raman Systems SPECTROSCOPY GROUP

Specifications Summary 1. Array Size (pixels) Pixel Well Depth (typical) 94,000 e - Dark Current 2. Read Noise 3

27 mm wide, 3 MHz Spectroscopy CCD. Spectroscopy at Pace. Specifications Summary 1. Register well depth:

Product Information Version 1.1. ZEISS Axiocam 702 mono Your 2.3 Megapixel Microscope Camera for Fast Low Light and Live Cell Imaging

26.6 x 3.3 mm / 1024 x 127 pixel Spectroscopy CCD. Specifications Summary 2. Active pixels 1024 x 127. Register well depth (typical) 1,000,000 e -

Specifications Summary 3. Active pixels 2048 x Pixel size (W x H) 13.5 x 13.5 µm. Active area pixel well depth (typical) 100,000 e -

Specifications Summary. Active pixels 1024 x Pixel size (W x H) 13 µm x 13 µm. Active area pixel well depth (typical) 100,000 e -

600 nm µm Spectroscopy InGaAs PDA. Specifications Summary. Active pixels 512 or Pixel well depth (typical)

ikon-xl 231 VERY LARGE AREA ASTRONOMY CCD P P P P CCD NEW

andor.com Scientific CMOS - Fast, sensitive, compact and light Features and Benefits Specifications Summary Ultra Sensitive Imaging Low Light Imaging

27 mm wide, 3 MHz Spectroscopy CCD. Spectroscopy at Pace. Specifications Summary 1. Register well depth:

26.6 x 3.3 mm / 1024 x 127 pixel Spectroscopy CCD. Specifications Summary 2. Active pixels 1024 x 127. Register well depth (typical) 1,000,000 e -

Wavelength (nm) Specifications Summary. Active pixels 512 x 512. Pixel size (W x H) 24 µm x 24 µm

4.2 Megapixel Scientific CMOS Camera

Goldeye G-032 SWIR Cool - low-noise short-wave infrared camera

TABLE OF CONTENTS PRODUCT DESCRIPTION CINCAM CCD TECHNICAL DATA SENSOR RESPONSE DIMENSIONS CINCAM CCD LARGE FORMAT TECHNICAL DATA SENSOR RESPONSE

High Resolution BSI Scientific CMOS

Specifications Summary 2

Neo scmos. Specifications Summary. Pixel size (W x H) 6.5 µm. Pixel well depth (typical) 25,000 e - Pixel readout rate (MHz) 560, 400, 200

Neo scmos. Specifications Summary. Pixel size (W x H) 6.5 µm. Pixel well depth (typical) 30,000 e - Pixel readout rate (MHz) 560, 200

hsfc pro 12bit ultra speed intensified imaging

Specifications Summary 3. Active pixels 2048 x Pixel size (W x H) 13.5 µm x 13.5 µm. Active area pixel well depth. Maximum readout rate

BSI scmos. High Quantum Efficiency. Cooled Scientific CMOS Camera

ASI178 Manual. Revision 1.2 Mar, 2018

dicam C4 intensified 16 bit scmos camera

dicam C1 intensified 16 bit scmos camera

PI-MAX4 Camera System

scmos discover new ways of seeing andor.com Features and Benefits Scientific CMOS - Fast, sensitive, compact and light. Specifications Summary

CMOS USORIA. Features

Back Illuminated Scientific CMOS

Specifications Summary. Active pixels 2048 x Active area pixel well depth 100,000 e - Maximum readout rate. Read noise 2.9 e - Maximum cooling

pco.edge electrons 2048 x 1536 pixel 50 fps :1 > 60 % pco. low noise high resolution high speed high dynamic range

Infrared Cameras. High Performance Cooled Infrared Cameras MWIR/LWIR/VLWIR Spectral Range Options SCIENTIFIC CAMERAS FEATURES

Goldeye G-033 TEC1. Description. Goldeye G High-speed VGA InGaAs camera. Benefits and features. Options

Leica DFC3000 G. Crisp fluorescence documentation for routine experiments

Eagle V. Models: EA4240-CL and EA4710-CL USER MANUAL

Goldeye G-032 TEC1. Description. Goldeye G VGA InGaAs camera with large pixel. Benefits and features. Options

Specifications Summary 2

ASI174 Manual. Revision 1.2 Nov, 2017

SWIR Vision Systems Acuros TM CQD TM SWIR Cameras. November 2018 SWIR VISION SYSTEM

FEATURES. APPLICATIONS Machine Vision Embedded Instrumentation Motion Control Traffic Monitoring Security

ASI071 Manual. Revision 1.3 Mar, 2018

ixon Specifications Summary Active pixels 128 x 128 Active area pixel well depth 250,000 e - Gain register pixel well depth 800,000 e -

ASI224 Manual. Revision 1.2 Mar, 2018

Goldeye CL-032. Description. Goldeye CL all purpose SWIR camera

ASI290 Manual. Revision 1.1 Nov, 2017

MonoVista CRS+ Raman Microscopes

Goldeye G-032. Description. Goldeye G all purpose short-wave infrared camera

Goldeye CL-008. Description. Goldeye CL High-speed, low-cost InGaAS camera

Specifications Summary. Active pixels 1024 x Pixel size (W x H) 13 µm x 13 µm. Active area pixel well depth

Versatile laser Raman Spectrometer. RMP-500 series

Prosilica GC 1380H. GigE Vision, Sony ICX285 EXview CCD sensor, auto-iris, 30 fps. Benefits and features: Options:

CMOS sensors are coming at age

Coherent kev Supercontinuum for Broad Element-Specificity. Courtesy of Dr. Daniil Kartashov. Specifications Summary 2. Register well depth

Datasheet Giganetix Board Camera GC2591M-BL GC2591C-BL

Transcription:

Powered by LightField The NIRvana: 64ST from Princeton Instruments is the world s first scientific grade, deep-cooled, large format InGaAs camera for low-light scientific SWIR imaging and spectroscopy applications. The camera uses a 64 x 512 InGaAs array with response from.9 mm to 1.7 mm. The detector is Peltier cooled to -6 C to minimize thermally generated noise and to improve signal-to-noise ratio for the most demanding SWIR applications. It offers 16-bit digitization and low read noise for outstanding dynamic range. FEATURE BENEFITS 64 x 512 InGaAs array High resolution imaging in the SWIR region; Offers 4X more pixels over 32 x 256 sensor 2 mm x 2 mm pixels High spatial resolution Response from.9 mm to 1.7 mm with 85% (typical) peak quantum efficiency Thermo-electric (Peltier) cooling Integrated cold-shield Electronic shutter C-mount Fused silica window GigE interface Optional: LightField for 64-bit Windows 7 Optional: WinView and WinSpec for 32-bit Windows XP/7 SITK for LabVIEW PICAM (64-bit)/PVCAM (32-bit) software development kits (SDKs) NIRvana: 64ST Excellent SWIR sensitivity for demanding imaging applications Minimizes dark noise and allows extended integration times without the need for liquid nitrogen; Built-in air or liquid cooling option for vibration sensitive environments Special cold shield limits the ambient thermal background Provides integration times from 2 ms to many seconds Standard lens interface compatible with numerous lenses and microscopes (spectrometer adapters available) AR coated, fused silica window for high transmission in SWIR range Industry standard for fast data transfer over long distances, up to 5 m Offers intuitive, cutting edge user interface; Provides data acquisition, defect correction, display and analysis Offers powerful, easy-to-use set of Windows GUI controls; Automates data acquisition, background and flat field corrections and display Easy integration into complex experimental setup Universal programming interfaces for easy custom programming; Compatible with Windows XP/7 (32-bit) and Windows 7 (64-bit) NIRvana: 64ST shown with lens, sold separately. Applications: Nanotube fluorescence, emission, absorption, non-destructive testing and singlet oxygen detection NOTE: Export of this camera outside of the United States is prohibited by law unless accompanied by a valid Export License as issued by the United States Department of Commerce. Page 1 of 5 NIRvana: 64ST Rev. N1

SPECIFICATIONS CCD image sensor CCD format CCD image area Pixel size Pixel well capacity (e - ) High Gain 4, 2D InGaAs focal plane array 64 x 512 imaging pixels 12.8 mm x 1.24 mm 2 mm x 2 mm High Capacity 6, Nominal gain (e - /count) 1 14 Typical system read noise (e - ) < 12 * (High Gain) Response nonlinearity: High gain < 2 ** % Cooling temp. @ +2 C ambient Cooling method -6 C (guaranteed), -65 C (typical with Air +15 C liquid circulation) Air only, liquid only, or a combination of air and liquid Dark current (e - /p/sec) @ -6 C ~ 15 Blemish specification Digitization Scan rate Frame rate Binning and ROI Cold shield Exposure time Window material Thermostating precision Operating temperature Certification Grade A: <2% defects For detailed blemish specifications, contact Princeton Instruments 16 bits 2 MHz, 5 MHz, 1 MHz 22 fps @ 2 MHz 55 fps @ 5 MHz 11 fps @ 1 MHz Software only f#/1.5 < 2 ms to >1 min Fused Silica (AR coated) ±.5 C across entire temperature range C to +3 C Weight / Dimensions (C-mount) 9.5 lbs (4.3 kg) / 7.4 x 5.8 x 5.8 (187.96 mm x 147.32 mm x 147.32 mm) (L x W x H) Weight / Dimensions (SP-mount) 9.5 lbs (4.3 kg) / 7.297 x 5.8 x 5.8 (185.34 mm x 147.32 mm x 147.32 mm) (L x W x H) CE * Measured with 1 µs exposure time ** Linearity for exposure > 2 ms All specifications are typical. Subject to change without notice. Page 2 of 5 NIRvana: 64ST Rev. N1

Sensor QE Curve 1 9 8 Quantum Efficiency (%) 7 6 5 4 3 2 1.8.9 1. 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 Wavelength (µm) NOTE: Graph shows typical Quantum Efficiency (QE) data measured at + 25 C. Longer cut-off wavelength shifts towards blue by 8 nm per every 1 C of cooling. Page 3 of 5 NIRvana: 64ST Rev. N1

IMAGING GROUP 2.9 2.35.75 19.5.75 19.5 2.35 2.9 2.9 2.35.476 12.8 1.755 44.58 1.725 43.82.62 15.74.625 15.88 NIRvana Drawing With C Mount 2.35 2.9 C-MOUNT THREAD 1.-2 UN 3.96 99.2 WINDOW FRONT SURFACE.351 8.91 4.63 2 UN THREAD 1.796 45.62 1.255 31.88.55 12.83.316 8.3 WINDOW IN VACUUM SURFACE.69 FPA LOCATION 1.15 29.21 3.13 79.53 LIQUID COOLANT INLET/OUTLET 7.4 187.84 7.62 193.66 NOTES: 1. ALL DIMENSIONS IN INCHES [MM] 2. WEIGHT: 9.5 LBS / 4.3 KGS 3. 4. 5. WINDOW THICKNESS =.125" [3.18MM] MECHANICAL SHUTTER NOT AVAILABLE MAX. POWER CONSUMPTION = 135W Spectrometer adapter is available upon request. Page 4 of 5 NIRvana: 64ST Rev. N1

IMAGING GROUP 3.6 91.45 B.C. 17.5 35 2X 1-32 UNF TYP. ALL FOUR SIDES 2.9.59 14.99 FPA DISTANCE.75 19.5.75 19.5 2.9 2.9 2.9 3.96 99.2 1.125 28.58 1.125 28.58 1.796 45.62 1.255 31.88.55 12.83.316 8.3.63.252 6.41 FRONT SURFACE OF VACUUM WINDOW 1.5 26.67 3.32 77.2 7.297 185.33 7.526 191.16 1.755 44.58 1.725 43.82.62 15.74.625 15.88 NIRvana Drawing With Spectrometer Mount 4.2 16.68 COOLANT INLET/OUTLET NOTES: 1. ALL DIMENSIONS IN INCHES (MM) 2. 3. 4. 5. WEIGHT: 9.5 LBS / 4.3 KGS WINDOW THICKNESS =.125" [3.18MM] MECHANICAL SHUTTER NOT AVAILABLE MAX. POWER CONSUMPTION = 135W C-mount adapter is available upon request. www.princetoninstruments.com info@princetoninstruments.com TOLL-FREE +1.877.474.2286 PHONE +1 69.587.9797 Visit the Princeton Instruments website to find a dealer in your area. Page 5 of 5 NIRvana: 64ST Rev. N1