|
Cesium Telluride Windowed Photodetectors
Cesium telluride (CsTe) photodetectors with magnesium fluoride (MgF2)
windows are issued by NIST as transfer
standard detectors in the spectral region extending from 116 nm to
254 nm. The photocathode is a semitransparent film of cesium telluride
which emits photoelectrons when exposed to ultraviolet radiation. The
cesium telluride film is deposited onto a MgF2 window and then mounted
on a ceramic body tube and sealed with an indium eutectic alloy. The entire
fabrication process is carried out under ultra high vacuum, and the interior
of the ceramic tube remains under vacuum for the lifetime of the detector.
The ceramic body has three electrical contact rings on it: one for the
photocurrent from the CsTe film, one for guarding against
leakage currents from the anode to the cathode, and one for the anode connection.
The sensitivity of a windowed photodetector is typically 0.05 to
0.20 electrons / photon throughout the calibration region from
116 nm to 254 nm. Calibration uncertainties (2-sigma) are 2% over
most the calibration region, but reach 9% at the shortest wavelengths. These
detectors have significantly reduced response to visible radiation (two or
more orders of magnitude lower than the ultraviolet response), and are
insensitive to radiation with wavelengths shorter than the MgF2
absorption edge around 113 nm. They offer extremely low dark current and
noise characteristics. However, the device efficiency may be degraded if the
window becomes contaminated in the user's vacuum system or darkens from
exposure to radiation in the MgF2 absorption region (wavelengths
less than 113 nm).
A fee schedule and ordering information are available.
In addition to these CsTe detectors, the
Vacuum UV
Transfer Standard Program issues other types of transfer standard detectors:
Detector Construction and Circuit Schematic
Radiation incident on the photocathode through the
MgF2 window generates photoelectrons in the cathode. An anode
biased 150 V above ground generates an electric field that enhances
the emission of electrons from the film.
Typical Efficiency of a NIST CsTe Transfer Standard
Detector efficiency is expressed in terms of electrons per
incident photon, and is a function of the incident radiation's wavelength.
|