A\ ANTES enlightening spectroscopy AVANTES EVO SERIES THE NEXT EVOLUTIONARY STEP FOR SPECTROMETRY

Avantes is proud to announce the latest additions to our EVO series spectrometers in UV/VIS and NIR range: EVO series; why? With the introduction of the AS7010 electronics board, Avantes brought new and improved functionality to their spectrometers. This Electronics board brings USB3 and ETHernet communication options to you. This is enabling faster data speeds, longer distances and network integration for your application. Improved electronics delivers more noise-free signals for your measurements and the on-board memory capabilities ensure plenty of capabilities for future features. Spectrometers...

EVO series in our Product Lines Productlines USB 3.0 Gigabit Ethernet More memory A/antes enlightening spectroscopy

EVO Series, with CMOS detector: StarLine AvaSpec-ULS2048CL-EVO Spectrometer Using CMOS technology instead of the conventional CCD technology, this spectrometer offers you the latest technology. New technologies like CMOS have evolved and become a suitable alternative. In combination with our latest AS-7010 electronics it offers you a versatile device including USB3.0 Communication with 10x higher speed compared to USB2, and a second communication port which offers Gigabit Ethernet for integration in your company network and possibility for long distance communication. Besides the high speed communication...

Order code UV/VIS/NIR UV/VIS/NIR UV/VIS UV UV UV UV UV/VIS VIS/NIR VIS VIS VIS VIS NIR NIR NIR NIR NIR * depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select. ** please note that not all 2048 pixels will be used for the useable range * depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the better the resolution Options • Replaceable slit • Quartz Detector Collection Lens (200-1100 nm) • Slit size, please specify XX = 5, 10, 25, 50, 100, 200 or 500 pm •...

EVO Series, with 4k CMOS detector: StarLine AvaSpec-ULS4096CL-EVO Spectrometer Another new member in our new EVO series: the AvaSpec-ULS4096CL-EVO. Using CMOS technology instead of the conventional CCD technology, this spectrometer offers you the latest technology; ready for the next decade. The dominant position of CCD detectors in the spectrometer field is fading and new technologies like CMOS have evolved and become a suitable alternative. The AvaSpec-ULS4096CL-EVO offers you this latest technology ensuring a spectrometer platform for the coming years. In combination with our latest AS-7010 electronics...

Order code UV/VIS/NIR UV/VIS/NIR UV/VIS UV UV UV UV UV/VIS VIS/NIR VIS VIS VIS VIS NIR NIR NIR NIR NIR * depends on the starting wavelength of the grating; the higher the wavelengt! ** please note that not all 4096 pixels will be used for the useable range UA UNA-DB | UB UC UD UE I UF BB VA VB VC VD I VE NB NC SI IA IB r the dispersion and the smaller the range to select. : depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the better the resolution Options • Replaceable slit • Quartz Detector Collection Lens (200-1100 nm) • Slit size,...

Unique is the second communication port which offers Gigabit Ethernet for integration in your company network and possibility for long distance communication.. This unique, first to the market combination enables you to create high speed multichannels systems, perfectly suited for most industrial applications. Options include a deep-UV detector coating, for better performance in the deep- UV-range, a detector collection lens to enhance sensitivity in the 200-1100 nm range and order-sorting filter to reduce 2nd order effects. Furthermore, the AvaSpec-2048L is available with a wide range of slit...

Order code UV/VIS/NIR UV/VIS/NIR UV/VIS UV UV UV UV UV/VIS VIS/NIR VIS VIS VIS VIS NIR NIR NIR NIR NIR UA UNA-DB | UB UC UD UE I UF BB VA VB VC VD I VE NB NC SI IA IB * depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select. ** please note that not all 2048 pixels will be used for the useable range Resolution table (FWHM in nm) for AvaSpec-ULS2048L-EVO Grating (lines/mm) This first to the market combination enables you to create high speed multichannel systems * depends on the starting wavelength of the grating;...

AvaSpec-HERO SensLine The AvaSpec-Hero is the top of the line spectrometer! Based on High Sensitivity Compact optical bench (f=100mm; NA=0.13) and a 1024x58 backthinned CCD detector, it offers the best of both worlds: Sensitivity and Resolution! The instrument is equipped with a TE Cooling enabling long integration times in low light applications. In conjunction with our AS7010 electronics, including a high end AD convertor, noise is kept to a minimum, which offers you an excellent Signal to Noise and Dynamic Range performance. From low light fluorescence applications to demanding Raman applications,...

Order code UV/VIS/NIR UV/VIS/NIR VIS/NIR UV/VIS VIS/NIR VIS/NIR UV/VIS VIS/NIR UV/VIS * depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select. Resolution table (FWHM in nm) for AvaSpec-HSC1024x58TEC-EVO Grating (lines/mm) 300 400 600 830 1200 2400 * Above values are average values. Due to optical properties resolution will be better in the lower wavelengths than in the higher wavelength range. • Replaceable slit with SMA connector, specificy slit size XX=10, 25, 50, 100, 200 or 500 pm. • As SLIT-XX-RS, but with...

Spectrometers AvaSpec-ULS2048XL-EVO SensLine High UV- and NIR-sensitivity back-thinned CCD Spectrometer Combining exceptional quantum efficiency with high-speed is the value proposition of the AvaSpec-ULS2048XL-EVO spectrometer. Unlike many back-thinned CCD spectro-meters, which have two dimensional arrays, the ULS2048XL-EVO has large monolithic pixels of 14x500 microns with exceptional efficiency in the UV, from 200400 nm, and the NIR, from 950-1160 nm. The instrument also has an electronic shutter, which enables integration times as low as 2 microseconds. To further enhance sensitivity, a detector...