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          NIRQuest光譜儀  IfyouutilizeNIRspectroscopyforresearch,processordiagnostics,NIRQuestisalesscostly,lesscomplexalternativetoFT-IRandcomparabletechnologies

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          NIRQuest 光譜儀

            If you utilize NIR spectroscopy for research, process or diagnostics, NIRQuest is a less costly, less complex alternative to FT-IR and comparable technologies.

            NIRQuest delivers a high-performance optical bench with low-noise electronics and more grating options than we've ever offered.

            This compact, multi-interface spectrometer is available in version for 900-1700 nm, 900-2050 nm, 900-2200 nm and 900-2500 nm.

            NIRQuest's modular design delivers more customization for a wider variety of applications including medical diagnostics, pharmaceuticals analysis, environmental monitoring and process control.

            NIRQuest for Laser Analysis

            NIRQuest is versatile enough to be configured for high-resolution laser and optical fiber characterization. The NIRQuest delivers reliable optical resolution to <0.25 nm (FWHM) and is easily customized for your high-resolution spectral applications.

            Thulium Fiber Laser

            Courtesy of Townes Laser Institute at the University of Central Floridas College of Optics & Photonics

            Turn NIRQuest into a Network Spectrometer

            When purchased with the Remora Network Adapter users can communicate with the NIRQuest over Ethernet or Wi-Fi. Use with SpectraSuite Software, and turn your device into a network accessible spectrometer. Remotely capture spectral data from anywhere Plus, Remora allows multiple users to access data and experiment settings without the need for additional equipment. Remora's web-interface works with all popular web browsers and allows you to monitor data from a PDA, iPhone, and most internet ready devices. - Learn more

          At a Glance

          NIRQuest512NIRQuest512-2.2NIRQuest256-2.1NIRQuest256-2.5
          Detector:Hamamatsu G9204-512 InGaAs linear arrayHamamatsu G9204-512W InGaAs linear arrayHamamatsu G9206-256 InGaAs linear arrayHamamatsu G9208-256 InGaAs linear array
          Detector Range:850-1700 nm900-2200 nm900-2100 nm900-2550 nm
          Useable range1:900-1700 nm900-2200 nm900-2050 nm900-2500 nm
          Pixels:512512256256
          Pixel size:25 m x 500 m25 m x 250 m50 m x 500 m50 m x 500 m
          Entrance aperture:
          25 m wide slit (standard); also, custom options (10, 50, 100 or 200 m wide slits) or fiber (no slit)
          25 m wide slit (standard); also, custom options (10, 50, 100 or 200 m wide slits) or fiber (no slit)
          25 m wide slit (standard); also, custom options (50, 100 or 200 m wide slits) or fiber (no slit)25 m wide slit (standard); also, custom options (50, 100 or 200 m wide slits) or fiber (no slit)
          Fiber optic connector:SMA 905SMA 905SMA 905SMA 905
          Grating options (standard):Grating NIR3, 150 l/mm, 900-1700 nmGrating NIR2, 100 l/mm, 900-2050 nmGrating NIR2, 100 l/mm, 900-2050 nmGrating NIR1, 150 l/mm, 1075-2500 nm
          Grating options (custom):Gratings NIR10, NIR11, NIR12, NIR13 and NIR14Gratings NIR2, NIR3, NIR10, NIR11, NIR12 and NIR13Gratings NIR2, NIR3, NIR10, NIR11, NIR12 and NIR13Gratings NIR2, NIR3, NIR10, NIR11, NIR12 and NIR13
          Longpass filter2:OF1-RG830 longpass NIR filter (optional)OF1-RG830 longpass NIR filter (optional)OF1-RG830 longpass NIR filter (optional)OF1-RG830 longpass NIR filter (optional)
          Wavelength range:900-1700 nm 
          w/Grating NIR3
          900-2150 nm 
          w/Grating NIR2
          900-2050 nm 
          w/Grating NIR2
          900-2500 nm 
          w/Grating NIR1
          Optical resolution (FWHM)3:~3.1 nm w/25 m slit~4.6 nm w/25 m slit~7.6 nm w/25 m slit~ 9.5 nm w/25 m slit
          Signal-to-noise ratio at full signal4:>15000:1 @ 100 ms integration
          >13000:1 @ 1000 ms integration
          >10000:1 @ 100 ms integration10000:1 @ 100 ms integration7500:1 @ 10 ms integration
          A/D resolution:16-bit16-bit16-bit16-bit
          Dark noise:6 RMS counts @ 100 ms
          12 RMS counts @ 
          1000 ms
          6 RMS counts @ 100 ms
          12 RMS counts @ 
          250 ms
          6 RMS counts @ 100 ms
          12 RMS counts @ 250 ms
          8 RMS counts @ 10 ms
          12 counts RMS @ 30 ms
          Dynamic range:15 x 10^6 (system); 5000:1 for a single acquisition15 x 10^6 (system); 1000:1 for a single acquisition5 x 10^6 (system); 5000:1 for a single acquisition3  x 10^5  (system); 5000:1 for a single acquisition
          Integration time5:1 ms-10 seconds1 ms-2000 ms1 ms-2000 ms1 ms-60 ms
          Corrected linearity:>99.8%>99.8%>99.8%>99.8%
          Computer interfaces:
          USB 2.0 @ 480 Mbps; RS-232 (2-wire) @ 115.2 K baud
          Wireless (Wi-Fi) interface:
          Yes, with Remora adapter
          Wi-Fi range:
          25 meters in free space

          1 Useable range?is defined in the context of the NIRQuest models detector response and its typical grating response. For example, the 512-element detector has response at 850 nm, but grating response begins at 900 nm. The G9206 256-element detector response is sensitive to TEC temperature, and has response only to 2050 nm when the TEC is set to -20 C. The G9208 256-element detector has response to 2550 nm, but the grating efficiency drops off at 2500 nm.
          2 Other filter options are available for order-sorting in the NIRQuest256-2.1 and NIRQuest256-2.5. Please contact an Applications Scientist for details.
          3 Optical resolution (FWHM) depends on grating and slit selection.
          4 SNR will decrease at longer integration times.

          5 Maximum integration times are defined as the longest amount of time one can integrate the spectrometer before the dark level rises to half of full scale.
           


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