*Photosensors* or *photodetectors* are [sensors|http://en.wikipedia.org/wiki/Sensors] of [light|http://en.wikipedia.org/wiki/Light] or other [electromagnetic|http://en.wikipedia.org/wiki/Electromagnetic_radiation] energy. There are several varieties:\[[1]\|http://en.wikipedia.org/wiki/Photodetector#cite_note-0\] |
[Cryogenic detectors|http://en.wikipedia.org/wiki/Cryogenic_detectors] are sufficiently sensitive to measure the energy of single x-ray, visible and near infra-red photons\[[2]\|http://en.wikipedia.org/wiki/Photodetector#cite_note-1\]. |
[Charge-coupled devices|http://en.wikipedia.org/wiki/Charge-coupled_device] (CCD), which are used to record images in [astronomy|http://en.wikipedia.org/wiki/Astronomy], [digital photography|http://en.wikipedia.org/wiki/Digital_photography], and [digital cinematography|http://en.wikipedia.org/wiki/Digital_cinematography]. Although before the 1990s [photographic plates|http://en.wikipedia.org/wiki/Photographic_plate] were the most common in astronomy. Glass-backed plates were used rather than film, because they do not shrink or deform in going between wet and dry condition, or under other disturbances. Unfortunately, [Kodak|http://en.wikipedia.org/wiki/Eastman_Kodak] discontinued producing several kinds of plates between 1980 and 2000, terminating the production of important sky surveys.\[[3]\|http://en.wikipedia.org/wiki/Photodetector#cite_note-2\] The next generation of astronomical instruments, such as the [Astro-E2|http://en.wikipedia.org/wiki/Astro-E2], include cryogenic detectors. In experimental [particle physics|http://en.wikipedia.org/wiki/Particle_physics], a [particle detector|http://en.wikipedia.org/wiki/Particle_detector] is a device used to track and identify elementary particles. |
The PDA series of Amplified Photodetectors integrates a wide range of photodiodes with an amplifier into compact packages. The modules possess a thin profile to allow access to light paths with the minimum amount of interference. All connections and controls are located perpendicular to the light path, providing increased accessibility. The low noise transimpedance or voltage amplifiers are capable of driving 50 Ω loads. All units include a removable threaded coupler that is compatible with many Thorlabs SM1 and SM05 threaded accessories. This allows convenient mounting of external optics, optical fibers, and apertures, as well as providing an easy mounting mechanism when using Thorlabs cage assembly accessories. Each housing provides two 8-32 tapped mounting holes (M4 for - EC versions) centered on the detector surface. A 120 VAC AC/DC power supply is included (230 VAC for - EC versions).
Please Note: Due to limitations in the IC, the high speed amplifier used in these devices may become unstable, exhibiting oscillations or negative output, if the power supply voltage is applied when the module is on. The unit should always be powered up using the power switch on the power supply or the unit itself. Hot plugging the unit is not recommended.