Ames Photonics: Modular Tools for Spectroscopy
LARRY USB2000 and LARRY USB4000 series: Scientific-grade CCD Linear Array Detectors
The LARRY USB series is a family of linear CCD array detectors that offers cost-effective, scientific-grade performance for a wide range of spectroscopic applications. They can be mounted to most spectrographs that have the output plane ≥10 mm outside of the spectrograph. Both standard and custom mounts are available, making them ideal for upgrading existing systems or incorporation into flexible new spectroscopic instruments.
The LARRY USB series is a custom build based on proven Ocean Optics electronics and is compatible with Ocean Optics software, enabling a broad scope of features. The detectors connect to and are controlled by a PC via USB 2.0, allowing for easy-to-use, plug-and-play operation. Multiple detectors can be controlled in the same software, enabling simultaneous acquisition. GPIO communication can also be used to integrate with other instruments and devices.
The linear CCDs used in the LARRY USB series contain on-chip electronic gating, which allow for integration times down to 1 ms without the need for external shutters.
Download datasheet here.
KEY FEATURES
- 2048 or 3648 pixel linear arrays
- 14 μm and 8 μm pixel width and pitch
- 200 μm pixel height for spectroscopic applications
- Scientific grade, no fringing
- Fast, on-chip electronic gating capability
- Maximum dynamic range >2000:1
- 200-1100 nm spectral range
- Low noise, uncooled
- Rapid acquisition up to 500 acquisitions / sec with 1 ms integration time
- USB 2.0 for full plug-and-play PC control
- Powered via USB
- GPIO for easy integration with other instruments and devices
- External trigger and sync output via SMB with programmable delays for synchronization to pulsed sources
- LARRY USB4000 has optional shutter mode, allowing integration times to 10 μs
APPLICATIONS
- Upgrade optical spectrometers to linear CCD array capability
- Capturing spectra of short-pulse events
- Synchronization to pulsed lasers and light sources
- Fringe analysis, beam profiling/monitoring
- Synchronous and simultaneous detection with multiple detectors
- General purpose linear detector, with Thorlabs cage mount interface available
CONNECTORS
- USB 2.0 for computer control and power supply
- Trigger SubMiniature BNC (SMB), TTL input for external trigger
- Sync SMB, programmable TTL output for synchronizing other devices with the detector
- Additional SMB connector for a customizable connection
- 22-pin accessory connector for detector monitoring and GPIO communication
PRICING:
LARRY USB2000: US$1,990 for base unit.
For further pricing details, please contact us.
SPECIFICATIONS | LARRY USB2000 | LARRY USB4000 |
Number of sensitive pixels | 2048 | 3648 |
Number of masked dark pixels | 18 | 13 |
Pixel size | 14 μm (w) × 200 μm (h) | 8 μm (w) × 200 μm (h) |
Array length (active) | 28.7 mm | 29.1 mm |
Spectral range | 200 nm – 1100 nm | |
Integration time | 1 ms – 65 sec | 3.8 ms – 10 sec 10 -1000μs option also available1 |
Well capacity (WC) | 62,500 e- | 100,000 e- |
16-bit ADC output | 65,535 counts | |
Saturation level @ 633 nm | 3.8 nJ/cm2 1.1 × 10-4 nJ per pixel |
9.5 nJ/cm2 1.5 × 10-4 nJ per pixel |
Readout noise (RN) | 29 e- rms | 46 e- rms |
Dark signal non-uniformity 1-sec integration 10-sec integration |
37 e- rms 406 e- rms |
571 e- rms 1739 e- rms |
Dark signal offset | ~1000 counts | |
Dark noise 1-sec integration 10-sec integration |
31 e- rms 45 e- rms |
69 e- rms 128 e- rms |
Maximum dynamic range (WC / RN) |
2155 | 2170 |
Readout time | 2 ms | 3.8 ms |
Spectral rate2 Normal High-speed acquisition |
Up to 30 Hz Up to 500 Hz |
Up to 30 Hz Up to 125 Hz |
External trigger jitter | ±420 ns | ±250 ns |
Power | Powered by USB or from accessory connector | |
Mounting | Ø42.5 x 6 mm mounting boss Detector located 9.5 mm below boss surface |
|
Connectors | USB 2.0, 480 Mbps SMB: External trigger input (TTL) SMB: Sync output (TTL) SMB: NC / customizable connection 22-pin accessory connector: Monitoring and GPIO |
Typical performance shown.
1Shorter integration times, down to 10 μs, possible with an alternative software package (Ocean View). Please contact us if you require this option.
2Spectral rate is based on Ocean Optics SpectraSuite software, and may depend on the PC specifications and configuration. Eliminating unnecessary background processes is recommended for high-speed operation. High-speed acquisition mode does not support multiple detectors.