It’s 2023 and tradeshows and conferences are starting back up. Some people are excited about the opportunity while others are reluctant to travel and meet face-to-face. StellarNet is now offering a virtual exhibition and spectroscopy hangouts in our new StellarLAB. Meet our team of scientists and engineers and discuss your application
Meet our StellarNet Team of Spectroscopy Experts!
Hear What People are Saying About our New Technologies!
“We have some really amazing new products right now! Out of all of them, I am the most excited about the Quasar Raman spectrometer because of its new high throughput design, which allows for 10X more photon collection! This makes it capable of being 10x faster, reducing noise, and increasing detection limits. Contact me to schedule a demo so that you can see the difference for yourself!” – Lady Light
“I am excited about our new RED-Wave offerings! We now have a ton of new extended range InGaAs models to choose from and these new detectors are more sensitive than ever! They can even be used for radiometry out to 2500nm! Less noise, more range (900-2500nm), more sensitivity… what could be better?” – Dark Noise
“I have been looking to add a SMA-locking mechanism to our instruments for years, but an elegant solution hadn’t popped up until now” – Beam Badger
New Quasar High Throughput Spectrometer
The Quasar comes with our new high throughput f/2 optical design for Raman spectroscopy with increased photon collection over 10x! This translates into taking spectroscopic measurements 10x faster, reducing noise, and increasing detection limits astronomically.
| Quasar Raman Spectrometer | Wavelength Range (cm-1) | 10x Optical Gain | Resolution (cm-1) | Detector Cooler Package ~°C Below Ambient |
|---|---|---|---|---|
| Quasar-532 | 200-4,500 | Yes | 9 | TEC-1,15°C |
| Quasar-532-TEC-X2 | 200-4,500 | Yes | 9 | TEC-X2, 30°C |
| Quasar-532-UC | 200-4,500 | Yes | 9 | UltraCool Vacuum, 80°C |
| Quasar-TEC-638 | 200-4,040 | Yes | 8 | TEC-1,15°C |
| Quasar-TEC-638 | 200-4,040 | Yes | 8 | TEC-X2, 30°C |
| Quasar-TEC-638 | 200-4,040 | Yes | 8 | TEC-X2, 30°C |
| Quasar-TEC-785 | 200-2,750 | Yes | 4 | TEC-1, 15°C |
| Quasar-TEC-785 | 200-2,750 | Yes | 4 | TEC-X2, 30°C |
| Quasar-785-UC | 200-2,750 | Yes | 4 | UltraCool Vacuum, 80°C |
| Quasar-1064 | 200-2,250 | Yes | 11 | TEC-X2, 30°C |
Near-Infrared for All Wavelengths
Your favorite StellaNet NIR spectrometers are now available in new flavors. Our most popular and highest-performing DWARF-Star range of 900-1700nm is now joined with several other RED-Wave extended range NIR spectrometers to suit all your NIR application needs.
RED-Wave Extended Range NIR Spectrometer
| Model | Wavelength Range (nm) | InGaAs Pixels | Grating g/mm | Estimated Resolving Resolution (nm) |
|---|---|---|---|---|
| NIR1.85 | 900-1850 | 512 | 300 | <13 |
| NIR2.15 | 900-2150 | 512 | 300 | <13 |
| NIR2.2 | 900-2300 | 512 | 300 | <13 |
| NIR2.2X | 1500-2200 | 512 | 600 | 7 |
| NIR2.2-1024 | 900-2200 | 1024 | 300 | 7 |
| NIR2.2X-1024 | 1500-2200 | 1024 | 600 | 2.8 |
| NIR2.5 | 1050-2500 | 512 | 300 | <15 |
StellarPro Software!
Drum roll, please… now combining features of your favorite SpectraWiz software with advanced tools and an App style interface, be prepared to have your mind blown. Built-in apps for Radiometry, Colorimetry, Chemical Absorption, and Kinetics are just a start. Our new StellarPro software also has integrated spectral preprocessing such as baseline subtraction, spike removal, and derivative view. Spectral ID matching, PLS Calibration model development, and run-time deployment are all included in this new software suite. StellarPro has user permission settings, login, and reporting to export all of your data in one place. Additional apps for Haze, Thin Film Analysis and more are also included!
Radiometry
App
Multichannel
App
Colorimetry
App
Haze
App
Absorbance
App
Thin-Film
App
Chemometrics
App
App
Settings
Spectral ID
App
User
Settings
SMA-Lock Spectrometer Input
Introducing our new keyed spectrometer and fiber optic cable locking system to allow repeatable placement of the fiber optic tip to the spectrometer entrance slit placement. Minor variations due to fiber optic adjustment can be reduced to <2%.
Join the StellarNet 2023 Virtual Exhibition and Spectroscopy Hangouts
If you are interested in learning about spectroscopy and see our spectrometers in action, please fill out the form below. We will schedule you in the next available StellarLAB DEMO time slot.