RAMaker
Your Vision, Our Mission.
Breakthroughs Made Real.
RAMaker
Your Vision, Our Mission.
Breakthroughs,
Made Real.

RAMaker
The RAMaker platform is where your most complex challenges are solved. We co-create the custom spectroscopic system that makes your vision a reality.
Deep ultraviolet to near infrared
229, 248, 266 and 325 nm reach resonance conditions in wide-bandgap materials and separate sp2 from sp3 carbon. 1064 nm escapes the fluorescence that buries Raman signal in tissue, polymers and pigments. Each mounts externally, because no single optical train serves both ends of that range — UV and NIR each need their own objectives, gratings and detector.
Six wavelengths, one sample position
Three lasers inside the chamber and up to three more added, every one landing on the same spot without realignment.
Ten wavenumbers from the laser line
A customized Bragg filter set opens the region a 50 cm-1 cut-off hides entirely: lattice modes, layer breathing modes in two-dimensional stacks, and low-frequency collective modes.
Angle-Resolved Polarized Raman and PL Imaging
Two angles rotate through 360° under software control — the polarization angle and the laser incident angle — and the software searches for the best-signal or zero-signal orientation automatically. For highly crystalline samples and thin films that is what makes lattice orientation readable rather than inferred.
Lifetime, not only intensity
Time-resolved photoluminescence and FLIM from 200 ps to 1 s, on the same confocal stage as the Raman measurement, with picosecond sources at 375, 405, 440, 473, 488 and 640 nm.
The environment is part of the instrument
−196 °C to 1500 °C, vacuum, and four-point probe measurements taken during acquisition rather than before and after it — so the electrical state and the spectrum belong to the same moment.
0.3 cm-1 resolution
Reached by physical configuration — 750 mm focal length with the 3600 gr/mm grating — not by a software setting. At that order peaks separate that are otherwise reported, and published, as one.
How RAMaker compares with MRID
Both instruments use the same parallel optical design and the same automated switching. They differ in how far each can be configured.
| Requirement | MRID | RAMaker |
|---|---|---|
| Excitation wavelengths at one sample position | Two | Up to six |
| Wavelength range | 375–830 nm | 229–1064 nm |
| Lowest accessible Raman shift | 50 cm-1, edge filter | 10 cm-1, Bragg set |
| Spectral resolution | 1.8 / 1.3 cm-1 | 0.9 to 0.3 cm-1 |
| Spectrograph | Fixed focal length | 193–750 mm, up to four gratings |
| Detection | Single detector | Up to two, 200–2500 nm |
| Raman and PL, mapping, polarized imaging | Yes | Yes |
| Fluorescence lifetime, TRPL and FLIM | — | 200 ps to 1 s |
| Sample environment | Optional stages | −196 to 1500 °C, vacuum, four-point probe |
| How it is supplied | Configured product | Built to specification |
The Configuration Space
You don’t need a specification. Your mission is where we start.
