AvaSpec-ULS2048CL-EVO (CMOS)

Another member in our EVO series: the AvaSpec-ULS2048CL-EVO.

Using CMOS instead of the conventional CCD technology, this spectrometer is completely up to date and 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-ULS2048CL-EVO offers you this latest technology ensuring a spectrometer platform for the coming years.

 

Overview

AvaSpec-ULS2048CL-EVO (CMOS)

Another member in our EVO series: the AvaSpec-ULS2048CL-EVO.

Using CMOS instead of the conventional CCD technology, this spectrometer is completely up to date and 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-ULS2048CL-EVO offers you this latest technology ensuring a spectrometer platform for the coming years.

In combination with our latest AS-7010 electronics, the AvaSpec-ULS0248CL-EVO offers you a versatile device including USB3.0 communication with 10 times 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, all at an affordable price.

Besides the high-speed communication options, the EVO series spectrometers also offer a fast microprocessor and 50 times more memory capacity, which can help you to store more spectra onboard and realize more functionality.

Options include a detector collection lens to enhance sensitivity in the 200-1100 nm range and order-sorting filter to reduce second-order effects. Furthermore, the AvaSpec-2048CL is available with a wide range of slit sizes, gratings and fiber-optic entrance connectors.
It comes complete with AvaSoft-Basic software, USB cable and an extensive manual.

The AvaSpec-ULS2048CL-EVO is also available as OEM unit, bench-only or Rackmount version.

Specifications

Optical Bench: ULS Symmetrical Czerny-Turner, 75 mm focal length

Wavelength range: 200-1100 nm

Resolution: 0.06-20 nm, depending on configuration (see table)

Stray-light: 0.19-1.0%, depending on the grating

Sensitivity: 375,000 counts/µW  per ms integration time

Detector: CMOS linear Image Sensor

Signal/Noise: 300:1

AD converter: 16 bit, 6 MHz

Integration time: 30 µs – 59s

Interface: USB 3.0 high speed, 5 Gbps / Gigabit Ethernet 1 Gbps

Sample speed with on-board averaging: 0.38 ms /scan

Data transfer speed: 0.38 ms /scan (USB3) / 1.0 ms (ETH)

Digital IO: HD-26 connector, 2 Analog in, 2 Analog out, 13 Digital bidirectional, trigger, sync., strobe, laser

Power supply: Default USB3 power, 500 mA / Or 12 VDC, 300 mA

Dimensions, weight: 177 x 127 x 44,5 mm (1 channel), 1135 grams

Use Useable range Spectral range (nm) Lines/mm Blaze (nm) Order code
UV/VIS/NIR 200-1100** 891** 300 300 UA
UV/VIS/NIR 200-1100** 891** 300 300/1000 UNA-DB
UV/VIS 200-850 515 600 300 UB
UV 200-750 247-218* 1200 250 UC
UV 200-650 163-143* 1800 UV UD
UV 200-580 113-69* 2400 UV UE
UV 200-400 69-45* 3600 UV UF
UV/VIS 250-850 515 600 400 BB
VIS/NIR 300-1100** 792** 300 500 VA
VIS 360-1000 495 600 500 VB
VIS 300-800 247-218* 1200 500 VC
VIS 350-750 142-89* 1800 500 VD
VIS 350-640 74-49* 2400 VIS VE
NIR 500-1050 495 600 750 NB
NIR 500-1050 218-148* 1200 750 NC
NIR 600-1160 346-297* 830 800 SI
NIR 600-1100** 495** 300 1000 IA
NIR 600-1100 495 600 1000 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

 

Slit size (µm)
Grating (lines/mm) 10 25 50 100 200 500
300 1.0 1.4 2.5 4.8 9.2 21.3
600 0.40-0.53* 0.7 1.2 2.4 4.6 10.8
830 0.32 0.48 0.93 1.7 3.4 8.5
1200 0.20-0.28* 0.27-0.38* 0.52-0.66* 1.1 2.3 5.4
1800 0.10-0.18* 0.20-0.29* 0.34-0.42* 0.8 1.6 3.6
2400 0.09-0.13* 0.13-0.17* 0.26-0.34* 0.44-0.64* 1.1 2.7
3600 0.06-0.08* 0.10 0.19 0.4 0.8 1.8

* Depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the better the resolution.

 

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