| Description | Andor’s TuCam is a new generation two-camera adapter for macro or microscopic imaging applications. Available in C- or CSUX-mount, TuCam features include large aperture, exceptional transmission, very low distortion and high precision alignment using kinematic cassettes.
Andor’s TuCam is a new generation two-camera adapter for macro or microscopic imaging applications. Available in C- or CSUX-mount, TuCam features include large aperture, exceptional transmission, very low distortion and high precision alignment using kinematic cassettes.
- Largest aperture
- High quality achromatic lenses
- Highest transmission
- Very low distortion
Bypass mode. Andor’s TuCam is a new generation two-camera adapter for macro or microscopic imaging applications. Available in C- or CSUX-mount, TuCam features include large aperture, exceptional transmission, very low distortion and high precision alignment using kinematic cassettes.
TuCam can be configured for simultaneous imaging from two similar cameras or as a switch between camera models with different imaging capabilities.
A full range of beam splitting optics are available with custom-designed kinematic cassettes for precision alignment. These include wavelength and polarization splitters of the highest quality as well as a first surface mirror for switching between cameras.
A variety of camera tubes & lenses is available to provide magnifications of 1.0x, 1.2x, 1.5x and 2.0x in each arm of the adapter. A filter wheel can also be integrated at the input of TuCam to enable pre-filtering of the desired emission band.... Read More | Balor is Andor’s game-changing, very large area sCMOS camera platform for Astronomy, the perfect solution for Large Sky Surveys that measure photometric and astrometric variability across timescales ranging from milliseconds to tens of seconds. | Inquire | Designed for very rapid imaging of low light events, combining > 500 frames/sec with single photon detection capability and > 90% Quantum Efficiency.
Thermoelectric cooling down to -100°C minimizes EM-amplified darkcurrent, whereas Andor’s ‘overclocked’ vertical shift speeds minimize both clock Designed for very rapid imaging of low light events, combining > 500 frames/sec with single photon detection capability and > 90% Quantum Efficiency.
Thermoelectric cooling down to -100°C minimizes EM-amplified darkcurrent, whereas Andor’s ‘overclocked’ vertical shift speeds minimize both clock induced charge noise and vertical smear during frame transfer.
The iXon3 860 Back-Illuminated EMCCD benefits from an advanced set of user–requested features, including OptAcquire, Count Convert, Spurious Noise Filters & Signal Averaging. RealGain™ provides quantitative EM gain calibration. Sub-millisecond biology is readily accessible through use of sub-array selection, pixel binning and Cropped Sensor Mode pushes frame rates to new extremes. The speed and sensitivity of the iXon3 860 Back-Illuminated EMCCD camera also renders it ideal for adaptive optics.
... Read More | ZL41 Wave is the next generation in the highly successful Zyla sCMOS series, specifically for physical science and astronomy researchers. Superb imaging and spectroscopic flexibility, compactness for tight optical spaces, extensive software compatibility and exceptional price/performance value.
ZL41 Wave is the next generation in the highly successful Zyla sCMOS series, specifically for physical science and astronomy researchers. Superb imaging and spectroscopic flexibility, compactness for tight optical spaces, extensive software compatibility and exceptional price/performance value.
Andor’s ZL41 Wave physical sciences sCMOS camera platform delivers sheer excellence in speed, sensitivity, dynamic range and resolution, with comprehensive imaging and spectroscopy functionalities. Building upon the strengths of the original Zyla sCMOS series, the cost-effective, compact, thermoelectrically cooled design of ZL41 Wave benefits from a reengineered and enhanced sensor chamber and is supported within a wide range of physical science software environments, integrating perfectly into any optical laboratory or observatory setting.
ZL41 Wave 4.2 provides exceptional sensitivity from a combination of 82% QE and very low 0.9 e- read noise from a 4.2 Megapixel sensor. Ideal for pushing frame rates in light starved applications within astronomy, quantum imaging, quantum computing, spectroscopy and 3D-tomography fields.
ZL41 Wave 5.5 is an ideal workhorse camera, a highly cost-effective and flexible solution that delivers a superior field of view from a 5.5 Megapixel sensor. Furthermore, this camera offers 2-in-1 rolling and true global shutter functionality. Global shutter is key to techniques such as particle imaging velocimetry (PIV) and astronomical object tracking.
ZL41 Wave sCMOS Features:
- NEW 32-bit binning mode - Access huge dynamic range through extensive pixel binning. User-selectable data bit-depth up to 32-bit, transmitted upstream over the camera interface.
- Spectroscopy mode - On-head asymmetric pixel binning and multitrack. Spectroscopist-friendly spectra and multi-track data, prior to transfer through 10-tap or USB interface. Upstream data size reduction and easier user data processing.
- Fast Spectroscopy: Up to 27,000 spectra/sec - Study of transient spectral phenomena with sub-millisecond time resolution.
- PIV capability (ZL41 Wave 5.5) - Perfect for fluid dynamics, Global Shutter mode of ZL41 Wave 5.5 facilitating image pair acqusition with an inter-frame gap of down to 100 ns.
- NEW Operate down to -20°C ambient temp - Ideal for use at higher elevation observatories under cold conditions.
- ZERO etaloning in the NIR - Front-illuminated sensor architecture, no unwanted signal modulation in the NIR compared to back-illuminated devices.
- GPU Express - Simplify and optimize data transfer from the camera - ideal for today's data intensive imaging experiments. Leverage CUDA-enabled NVidia GPU processing to accelerate the data acquisition pipeline.
- Linux, Windows, Labview and Matlab ready - Full and flexible SDK options for a wide variety of physical science laboratory and observatory uses.
- NEW Python ready - Python wrapper integration and full supporting documentation in latest camera SDK helps integration and full control of custom-build systems.
- NEW ASCOM, EPICS and Tango ready - Supported in open source software platforms. ASCOM astronomy instrument control standard; EPICS and Tango Lima are used for hardware control at a number of particle accelerators and large scientific instruments facilities worldwide.
- NEW Enhanced image quality - Updated QC processes ensure every ZL41 Wave delivers optimal image quality. Ultra-low Photon Response Non-Uniformity (PRNU) for clear, uniform images.
- NEW Enhanced sensor chamber - An updated sensor chamber provides even greater long-term protection from condensation in high humidity environments (3 year chamber warranty).
- 5.5 and 4.2 megapixel formats - Sharp resolution over a large field of view. Ideal for astronomy, area scanning applications or multi-track spectroscopy.
- QEmax up to 82% - Highest available photon capture efficiency across visible/NIR.
- ~ 1 e- Read Noise - Noise floor down to 0.9e- Lower detection limit than any CCD.
- 100 fps (Camera Link) - Zyla offers ‘10-tap’ Camera Link for maximum sustained frame rates.
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