Model 658 End-on PMT Housing Assembly

The photomultiplier tube (PMT) is among the most popular photosensitive devices. Various tube types and scintillator treatments permit use of these detectors from the Extreme Vacuum Ultraviolet (EUV) through the Visible and into the near Infrared. They provide large photosensitive areas, secondary emission multiplication (high gain), low dark noise and fast time response. Photomultipliers are ideal for a broad range of spectroscopy applications.
The Model 658 accommodates 28mm end on PMTs. All end-on photomultiplier housing assemblies are provided with a socket for a specified tube, tubes are specified separately. The housing has connectors for current output and high voltage (HV) input. Some models are equipped with scintillators for vacuum ultraviolet (VUV) operation. The scintillator converts invisible vacuum ultraviolet light to a Visible light emission, easily detected by sensitive PMTs. This detector housing assembly is available with 2.75" CF flange, NW40 Quik flange, and McPherson flange terminations.

Model 658 PMT Housing Assembly Data Sheet

See also PDF Sheet for the sodium salicylate scintillator and a guide to readily available coated windows


Additional Information:

Frequently Used End-on Photomultiplier (PMTs)
Type Range, nm Peak, nm Max. Vdc Sensitivity, uA/lm Typ Amplification Rise Time Transit Time
R6095 300 - 650 420 1500 88 2.1 x 10^6 4 ns 30 ns
R374 185 - 850 420 1500 64 5.3 x 10^5 15 ns 60 ns
Part Numbers for the Model 658 Photomultiplier Tube (PMT) Housing Assembly
Part NumberDescription
8105-0658-0 Model 658 Atmospheric photomultiplier tube detector housing (for end-on 28mm dia tubes) with magnetic shielding, dynode network and socket. Requires PMT. Provided with a mounting flange fitting McPherson slits.
8105-0658-1 Model 658 Vacuum photomultiplier tube detector housing (for end-on 28mm dia tubes) with magnetic shielding, dynode network and socket. Requires PMT. Provided with a mounting flange fitting McPherson slits and a scintillator coated window for use in the vacuum ultraviolet.
8105-0658-2 Model 658 Vacuum photomultiplier tube detector housing (for end-on 28mm dia tubes) with magnetic shielding, dynode network and socket. Requires PMT. Provided with a ISO NW40KF flange and a scintillator coated window for use in the vacuum ultraviolet.
100-110470 Model 658 UHV photomultiplier tube detector housing (for end-on 28mm dia tubes) with magnetic shielding, dynode network and socket. Requires PMT. Provided with a DN40CF scintillator coated window flange for use in the vacuum ultraviolet and UHV.
8446-1003-0 Replacement Sodium Salicylate coated window for Model 658
8446-1003-0 Replacement Sodium Salicylate coated window for ISO NW40KF terminated Model 658

Sample Spectra

example emission spectrum from the hollow cathode lamp

Outline Drawing

McPherson Model 658, Outline Drawing

Select Publications

Abstract: This paper is a report on our effort to use reflectance measurements of a set of amorphous silicon (a-Si) and uranium (U) multilayer mirrors with an uranium oxide overcoat to obtain the optical constants of a-Si and uranium. The optical constants of U, its oxides, and Si, whether crystalline or amorphous, at 30.4 and 58.4 nm in the extreme ultraviolet (EUV) are a source of uncertainty in the design of multilayer optics. Measured reflectances of multilayer mirror coatings do not agree with calculated reflectances using existing optical constants at all wavelengths. We have calculated the magnitude and the direction of the shift in the optical constants of U and a-Si from reflectivity measurements of DC magnetron sputtered a-Si/U multilayers at 30.4 and 58.4 nm. The reflectivity of the multilayers were measured using a UV hollow cathode plasma light source, a 1 meter VUV monochromator, a back-thinned CCD camera, and a channeltron detector. These reflectance measurements were verified by measurements made at LBNL. The reflectances of the multilayer coatings were measured at 14.5 degrees from normal to the mirror surface. The optical constants were calculated using IMD which uses CURVEFIT to fit the optical constants to reflectivity measurements of a range of multilayer mirrors that varied over a span of 150 - 25.0 nm bilayer thickness. The effects of surface oxide and roughness, interdiffusion, and interfacial roughness were numerically subtracted in fitting the optical constants. The (delta) , (beta) determined at 30.4 nm does not well match the values of c-Si published in the literature (HBOC1), but do approach those of a-Si as reported in literature (HBOC). The difference in the optical constants of c-Si and a-Si are larger than can be attributed to differences in density. Why the optical constants of these two materials vary at 30.4 remains an open question.
M. B. Squires, D. D. Allred, R. S. Turley

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