Full text loading...
No data available.
Please log in to see this content.
You have no subscription access to this content.
No metrics data to plot.
The attempt to load metrics for this article has failed.
The attempt to plot a graph for these metrics has failed.
Ge : Ga photoconductors in low infrared backgrounds
1.W. L. Hansen, Nucl. Instrum. Methods 94, 377 (1971),
1.E. E. Haller, W. L. Hansen, G. S. Hubbard, and F. S. Goulding, IEEE Trans. Nucl. Sci. NS‐23, 81 (1976).
2.E. E. Haller, Izv. Akad. Nauk SSSR, Phys. Series 42, 1131 (1978).
3.W. J. Moore and H. Shenker, Infrared Phys. 5, 99 (1965).
4.A. G. Kazanskii, P. L. Richards, and E. E. Hailer, Solid State Commun. 24, 603 (1977).
5.A. G. Kazanskii, P. L. Richards, and E. E. Haller, Appl. Phys. Lett. 31, 496 (1977).
6.E. L. Dereniak, R. R. Joyce, and R. W. Capps, Rev. Sci. Instrum. 48, 392 (1977), see Fig. 4.
7.Tests by J. R. Houck at the Astronomy Department, Cornell University, and by F. J. Low at the Lunar and Planetary Laboratory, University of Arizona, showed that our measurements of the current responsitivities of the two conventional detectors in Table I were conservative by factors of 1.5 and 1.2, respectively.
8.P. R. Bratt and N. N. Lewis, Development of Doped Germanium Photoconductors for Astronomical Observations at Wavelengths from 30 to 120 Micrometers, Santa Barbara Research Center, NASA CR‐152, 046, 1977 (unpublished).
9.G. E. Stillman, C. M. Wolfe, and J. O. Dimmock, in Semiconductors and Semimetals, edited by R. K. Willardson and A. C. Beer (Academic, New York, 1977), Vol. 12, p. 169.
Article metrics loading...