Micro Spectrophotometers

2030XL PRO™ Microspectrometer-Large Samples

The 2030XL PRO™ microspectrophotometer is designed to acquire spectra, images, and film thickness measurements of microscopic features of large scale samples. “XL” stands for “extra large” and these are the types of samples for which this instrument was built.

The 2030XL PRO™ microspectrophotometer allows you to measure UV-visible-NIR range transmission, absorbance, reflectance, emission and photoluminescent microspectra™ of features smaller than a micron across. Yet, depending upon the instrument configuration, the size of the sample can essentially be unlimited. Now you can map color variations within pixels of the biggest flat panel displays, measure film thickness of 300 mm wafers with ease or measure the fluorescence of the largest artworks.

Features

Microspot analysis of large scale samples
Spectral Range: 200 to 2500 nm
UV-visible-NIR transmission microspectroscopy
UV-visible-NIR transmission imaging
UV-visible-NIR reflectance microspectroscopy
UV-visible-NIR reflectance imaging
UV-visible-NIR fluorescence microspectroscopy
UV-visible-NIR fluorescence micro-imaging
Raman microspectroscopy
UV-visible-NIR photoluminescence microspectroscopy
UV-visible-NIR photoluminescence imaging
Polarization microspectroscopy in the UV, visible and NIR regions
Polarization microscale imaging in the UV, visible and NIR regions
Thin film thickness measurements
Colorimetry of microscopic samples
Manual or fully automated operation
Featuring Lightblades™ technology
Scorpii™ Advanced Illumination system
Integrated TE cooled array detectors available for low noise and long term stability
Precision temperature control of samples
Calibrated, variable measurement areas even smaller than a micron
Superior images both with eyepieces and digital imaging
Featured with Lambdafire™ spectroscopy and imaging control and analysis software.
Specialized software modules including statistical analysis, spectra mapping, spectral databasing, image analysis and more

508 PV™ M i c r o s c o p e Spectrophotometer

The 508 PV™ microscope spectrophotometer can easily be added to an existing microscope, probe station or even be used to upgrade an older microspectrophotometer. Depending upon the microscope configuration, you will then be able to take absorbance, transmittance, reflectance, polarization and even fluo- rescence microspectra™ of samples smaller than a micron. With CRAIC Technologies™ Universal Microscope Adapters, the 508 PV™ can be added to just about any microscope.

508 PV Specifications:

Spectrophotometer Range	200-900 nm 350-1000 nm 900-1700 nm 900-2100 nm
Fluorescence Excitation	365 to 546 nm
Laser Illumination	Available
Sampling Area	Variable from 1 to 10000 microns2
Spectral Resolution	User selectable from 1 to 15 nm
Detectors	CCD and InGaAs Arrays
Detector Cooling	Available
Scan Time (Full Range)	4 millisecond minimum
High Resolution Color Imaging	Included
Image Resolution	Up to 5 Megapixels
Programmable Stage with Mapping	Available
Operating System	Windows 7 Pro, Windows 8

Apollo™MicroRaman Spectrometer Module

The Apollo™ Raman spectrometer modules can be combined to offer several laser wavelengths on a single instrument. Each is permanently aligned so using the system is as simple as focusing on your sample. The system can be added to any CRAIC microspectrometer for a powerful, multi-purpose analytical tool.

Combined with CRAIC Technologies LambdaFire™ software, Apollo™ Raman microspectrometers can acquire single point spectra or, with an automated stage, create 3D Raman spectral maps. LambdaFire™ controls the instrument while offering many data analysis capabilities. This includes optional searchable libraries to aid in spectral identification.

Apollo™ Raman Features

405, 473, 488, 532, 638, 660, 785, 830nm lasers
Multiple lasers can be combined on single instrument
Permanently aligned for ease of use
Single point and Raman spectral mapping
Can be added to CRAIC microspectrometers
Can be added to many microscopes

APOLLO RAMAN Specifications:

Excitation Source
Wavelength (nm)	405, 473, 488, 532, 638, 660, 785, 830
Bandwidth	< 0.02 nm
Output Power	50-100 mW
Spectrometer
Spectral Range	120 to 3000 cm-1**
Spectral Resolution	6 cm-1
Sampling Area (20x)	14 um
Detectors
Type	TE cooled CCD
Integration Time	8 ms to 10 minute
A/D Resolution	16 bit
Dynamic Range	25000
Electronics
Interface	USB 2.0
Input power	110-220 VAC

CoalPro II™ – Optical Petrography System

The CRAIC CoalPro II™ system was designed to measure vitrinite reflectance accurately, rapidly, and nondestructively. The system combines research quality petrographic microscopes with Lightblades™ technology and a software package written specifically for petrographic analysis. The CRAIC CoalPro II™ system makes measurements per the ISO 7404-5 and ASTM D2798 standard test methods and presents the results in an in- dustry standard format including histograms. The system can even be automated with the inclusion of a programmable stages and point counting.

CoalPro II Features:

Easy, quick and accurate vitrinite reflectance
Automatic calibration and optimization
Automated or manual measurements
ISO 7404 & ASTM D2798 industry standard reports including histograms
Polarization imaging and microspectroscopy
Can measure vitrinite reflectance of even sub-micron samples

Lambdafire™ – Microspectrometer Software/ Reference Standards

Key Features

Microspectrophotometer Control and Data Analysis in one easy-to-use package
Microspectrophotometer automation control and programming
Data analysis features included with instrument control
Imaging control and analysis
Perfect for research as well as production with many features specific to both
Many plug-in modules available such as Spectral Surface Mapping™, thin-film thickness, colorimetry and more
Lambdafire™ is a native 64-bit application
Runs under Windows 10^®
Easy to use
From the experts in microspectroscopy