Details
The STS-UV-RAD (210-600 nm) is a radiometrically calibrated microspectrometer with direct-attach cosine corrector, and is ideal for irradiance applications including LED characterization. Its rugged design and great unit-to-unit reproducibility make STS-UV-RAD attractive for integration into high-volume applications such as LED sorting on a production line.
Overview
- Compact – actual size is 40 x 42 x 24 mm
- Powerful – high signal-to-noise (>1500:1) and dynamic range (4600:1) performance
- Thermally stable – peak shape stays the same over a wide temperature range
- Cost-effective – optical resolution of 1.5 nm is comparable to more expensive setups
- Reproducible – attractive design for integration and scalability
- Software – Oceanview Software is included
Specifications
Subject to change depending on model type
Detector:
- Detector:
- CMOS
- Entrance slit:
- 25 µm
- Detector Collection Lens:
- No
Physical:
- Dimensions:
- 40 mm x 42 mm x 24 mm
- Weight:
- ~ 60 g
Spectroscopy:
- Integration Time:
- 10μs - 10s
- Optical Resolution:
- 1.5 nm
- Wave Length Range:
- 210nm - 600nm
- Dark Noise:
- ≤3 counts RMS
- Dynamic Range:
- 5 x 109 (system, 10 s max integration), ~4600 single acquisition
- Signal to Noise Ratio:
- >1500:1 (full signal)
- Stray light:
- ≤0.25%
Follow these steps how to set up the OceanView software to measure successfully your lamp or light source output power
-
Item Code: WAVEGO-VIS-50
-
Item Code: FLAME-S-RAD
Accessories
-
Item Code: JAZ-CBL-DB15