Fig. 2 Transmittance spectra of BG36 Schott Glass Filter taken with the MS125™ Spectrograph used a 400 l/mm grating blazed at 500 nm, and a 50 µm input slit. Integration time = 50 ms, averaging = 1 and 500 (noted on the inset graph).Complete packages - Oriel MS125TM Spectrograph and linear array detector
2048 CCD linear array
True plug and play systems with USB interface
New intuitive spectrograph software
LineSpec Spectrometers are made up of our Oriel MS125™ 1/8 m spectrograph and an external 2048 CCD array. Gratings and slits are interchangeable so you can re-define the usable spectral range and resolution, as your needs change. We also offer the array detector separately, for mounting to other Oriel Spectrographs.
Complete systems include spectrograph, detector head with mounting flange, software, and your choice of grating and input slit.
The LineSpec Linear Array camera is a 2048 pixel CCD detector with LineSpec Basic software which can be integrated with various Oriel spectrograph models:
MS125™ Spectrograph
Your choice of grating
Your choice of entrance slit with input slit holder
2048 CCD detector with mounting flange
LineSpec™ Software and LabVeiw drivers included
We chose the MS125 as the spectrograph for these systems, because of its high resolution and throughput, economical price and compact size. The MS125 is a micrometer driven, 1/8 m (120 mm), focal length instrument.
Fig. 2 Transmittance spectra of BG36 Schott Glass Filter taken with the MS125™ Spectrograph used a 400 l/mm grating blazed at 500 nm, and a 50 µm input slit. Integration time = 50 ms, averaging = 1 and 500 (noted on the inset graph).
| Model | Description | Availability | Price | Qty. | |
|---|---|---|---|---|---|
| 78877 | Oriel LineSpec™ CCD Array Spectrometer, 2048 Pixel, 200-1100nm | Call | ¥53,517.88 | ADD |
| Grating Model | Line Density (I/mm) | Blaze Wavelength | Spectral Resolution (nm)* |
Array Bandpass (nm) |
Primary Wavelength Region (nm)** |
|---|---|---|---|---|---|
| 77419 | 2400 | 250 | 0.11 nm | 84 | 200 - 500 |
| 77411 | 1200 | 350 | 0.22 nm | 170 | 200 - 1000 |
| 77464 | 1200 | 500 | 0.22 nm | 170 | 280 - 1600 |
| 77412 | 1200 | 750 | 0.22 nm | 163 | 450 - 1000 |
| 77414 | 600 | 400 | 0.43 nm | 338 | 250 - 1300 |
| 77415 | 600 | 750 | 0.43 nm | 338 | 450 - 2000 |
* Measured with 10 µm x 2 mm slit and 2048 array detector.
** The primary wavelength region is where the grating efficiency is >20%. System efficiency will also be affected by the reflectivity of the spectrograph\'s mirrors and the grating angle, at any wavelength.
