The MS127i is a versatile, efficient, single grating, imaging spectrograph at an affordable price. For spectroscopy applications not covering a broad spectral range, and not requiring the resolution and imaging performance of our high end MS260iTM and MS257TM ¼ m instruments, the MS127iTM is the right choice. For a specification comparison of all our spectrographs, refer to Table 1.
Table 1 Oriel Spectrographs
|
Spectrograph |
Imaging |
Automated |
Spectral Resolution (nm)* |
No. of Gratings Supported |
Built-in Shutter |
Max No. of Fiber Tracks |
Dual Output Ports |
RS-232 |
IEEE-488 (GPIB) |
| Imaging Spectrograph, 1/8 m, Single Grating, Oriel MS127i |
X |
|
0.22 nm |
1 |
X |
5 |
|
|
|
| MS260i 1/4 m Spectrograph,GPIB, 1 Output Port, Grating & Slit Ordered Separately |
X |
X |
|
3 |
X |
9 |
|
Standard |
Standard |
| MS260i 1/4m Spectrograph,GPIB, 2 Output Ports, Grating & Slit Ordered Separately |
X |
X |
|
3 |
X |
9 |
X |
Standard |
Standard |
| MS257TM 1/4 m Monochromator, RS-232 |
|
X |
0.15 |
4 |
X |
1 |
X |
Standard |
Optional |
| MS257TM 1/4 m Imaging Spectrograph RS-232 |
X |
X |
0.15 |
4 |
X |
9 |
|
Standard |
Optional |
| MS125 Spectrograph, 1/8 m, Grating and Slit Ordered Separately |
|
|
0.22 nm |
1 |
|
1 |
|
|
|
Optical Configuration
The MS127i has been designed for ultra low stray light and no re-diffracted light. It utilizes a Czerny-Turner optical layout with one significant modification - the addition of an astigmatism correcting mirror after the collimating mirror (see Fig. 1). This patented system allows high spectral and spatial resolution at a low F/#, F/3.8.
Fig. 1 Optical configuration of MS127i 1/4 m Spectrograph
Wavelength Drive
Wavelength setting is manual on the MS127i. The instrument is calibrated for the central wavelength of the image field when using a 1200 l/mm grating. If you are working with a 2400, 600, 400, etc. l/mm grating, multiply the wavelength setting by the wavelength scale conversion factor listed in Table 2. Although the simple drive mechanism does not allow very accurate wavelength settings, it is highly reproducible and will allow you to switch between pre-determined wavelength positions with confidence.
Multi-track Spectroscopy with MS127i Spectrograph
Full correction for astigmatism in spectral instruments requires sophisticated toroidal mirrors (as in our MS257 1/4 m spectrograph); they allow vertical resolution of many tracks simultaneously. But, for many applications there is a need for only 2 to 3 tracks, as in double beam work. We designed the MS127i to correct astigmatism economically. You can reliably separate multiple tracks for Multi-track Spectroscopy with a CCD that has the ability to record individual tracks, such as our InstaSpec CCDs. Thus, MS127i makes the acquisition of double beam spectra of pulsed or continuous sources possible on a limited budget.
Built-in Shutter
A normally closed shutter located behind the input slit effectively blocks light from entering MS127i. The shutter circuitry is housed inside MS127i; shutter power is from a simple 5 V supply, provided. Minimum opening time is 0.2 s. This shutter will operate at rates to 0.5 Hz.
Interchangeable Gratings
We offer a large selection of interchangeable gratings for the MS127i. Choose the one that covers the spectral range of interest. The gratings are supported on a precision holder, which clips into the grating mount. They can be easily interchanged without the need to realign the instrument. Table 2 lists the specifications for each model.
Table 2 Gratings for MS127i 1/8 m Spectrograph
|
Model |
Line Density (I/mm) |
Blaze Wavelength |
Grating Type |
Wavelength Scale Conversion Factor |
Multichannel Array Bandpass (nm)* |
Spectral Resolution (nm)** |
Peak Efficiency (%) |
Primary Wavelength Region*** (nm) |
Instrument's Upper Mechanical Wavelength Limit (for specified grating) |
| 77483
|
3600 |
405 |
Holographic |
0.33 |
46 |
0.06 nm |
60 |
180 - 395 |
395 |
| 77484
|
2400 |
250 |
Holographic |
0.5 |
84 |
0.11 nm |
65 |
180 - 600 |
600 |
| 77485
|
2400 |
400 |
Holographic |
0.5 |
81 |
0.11 nm |
65 |
230 - 600 |
600 |
| 77486
|
1800 |
500 |
Holographic |
0.67 |
107 |
0.14 nm |
80 |
300 - 805 |
805 |
| 77487
|
1200 |
250 |
Holographic |
1 |
165 |
0.22 nm |
80 |
180 - 650 |
1200 |
| 77488
|
1200 |
350 |
Ruled |
1 |
165 |
0.22 nm |
80 |
200 - 1200 |
1200 |
| 77489
|
1200 |
750 |
Ruled |
1 |
163 |
0.22 nm |
80 |
450 - 1200 |
1200 |
| 77491
|
600 |
400 |
Ruled |
2 |
330 |
0.43 nm |
85 |
250 - 1300 |
2400 |
| 77492
|
600 |
750 |
Ruled |
2 |
2400 |
0.43 nm |
75 |
450 - 2400 |
2400 |
| 77473
|
600 |
1250 |
Ruled |
2 |
328 |
0.43 nm |
85 |
750 - 2400 |
2400 |
| 77474
|
600 |
1600 |
Ruled |
2 |
320 |
0.43 nm |
90 |
900 - 2400 |
2400 |
| 77493
|
400 |
350 |
Ruled |
3 |
493 |
0.65 nm |
65 |
200 - 800 |
3600 |
| 77494
|
400 |
500 |
Ruled |
3 |
495 |
0.65 nm |
80 |
300 - 1200 |
3600 |
| 77477
|
400 |
1600 |
Ruled |
3 |
498 |
0.65 nm |
85 |
900 - 2900 |
3600 |
| 77495
|
300 |
300 |
Ruled |
4 |
655 |
0.86 nm |
75 |
200 - 750 |
4800 |
| 77478
|
300 |
1000 |
Ruled |
4 |
655 |
0.86 nm |
85 |
575 - 2500 |
4800 |
| 77479
|
246.16 |
226 |
Ruled |
4.8 |
795 |
1.02 nm |
60 |
190 - 450 |
5760 |
Input Slits
MS127i comes with an input slit holder. We provide fixed slits in widths from 10 to 200 µm.
Mounting
MS127i has 1/4-20 tapped holes for rod mounting, or you can simply sit it on a flat surface. It is heavy enough to support a detector, without being hard mounted to a baseplate.
Specifications
| Input Focal Length |
127 mm |
| Exit Focal Length |
138.5 mm |
| F/# |
F/3.7 |
| Usable Wavelength Range |
180 nm to 25 µm with interchangeable gratings |
| Horizontal Magnification (Spectral Direction) |
1.1 |
| Vertical Magnification (Spatial direction) |
1.1 |
| Resolution |
0.22 nm* |
| Maximum Blur Size in Vertical Direction |
0.7 nm |
| Wavelength Accuracy |
1 nm** |
| Wavelength Scale Reproducibility |
0.1 nm*** |
| Weight |
8 lbs (3.6 kg) |
*With 1200 l/mm grating, 10 µm x 2 mm slit and 14 x 200 µm size pixels (2048 element array).
**Accuracy of wavelength scale, does not include the tolerance of the detector mounting.
***Reproducibility of wavelength calibration of the whole system, the spectrograph plus the detector, related to repetitive settings of the 1200 l/mm grating to the same position.