Application of Superconducting Hot-Electron Bolometer Mixers for Terahertz-Band Astronomy

Author:

MAEZAWA Hiroyuki1

Affiliation:

1. Osaka Prefecture University

Publisher

Institute of Electronics, Information and Communications Engineers (IEICE)

Subject

Electrical and Electronic Engineering,Electronic, Optical and Magnetic Materials

Reference66 articles.

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2. [2] D. J. Hollenbach and A. G. G. M. Tielens, “Dense photodissociation regions (PDRs),” Annu. Rev. Astron. Astrophys., vol.35, no.1, pp.179–215, Sept. 1997.

3. [3] D. C. Mattis and J. Bardeen, “Theory of the anomalous skin effect in normal and superconducting metals,” Phys. Rev., vol.111, no.2, pp.412–417, July 1958.

4. [4] Y. Uzawa, M. Kroug, T. Kojima, M. Takeda, M. Candotti, Y. Fujii, K. Kaneko, W. Shan, T. Noguchi, and Z. Wang, “A sensitive ALMA Band 10 SIS receiver engineering model,” Supercond. Sci. Technol., vol.22, no.11, pp.114002, Nov. 2009.

5. [5] J. J. A. Baselmans, A. Baryshev, S. F. Reker, M. Hajenius, J. R. Gao, T. M. Klapwijk, B. Voronov, and G. Gol'tsman, “Influence of the direct response on the heterodyne sensitivity of hot electron bolometer mixers,” J. Appl. Phys., vol.100, no.8, pp.084510, Oct. 2006.

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