NASA NTRS · 20130000256
Achieving BLISS: Challenges for Building Fast, Ultra-Sensitive Transition-Edge Sensors
Abstract
Topics: 1.Motivation and Intro to TESs. 2. BLISS Specifications-tolerance to dark power. 3.Measuring stray (dark) power-Tc (alpha) and G measurements. a) Overview two methods: JTD vs. TES. b) TES arrays: measurement and complications for Pd, Tc, and alpha. 4. Results: Pd compare, NEP, tau, 1/f issues. LIRGs and ULIRGs: Excellent example of distinct optical/UV and IR luminosity. Interaction long known, but huge luminosity is not predicted based on optical studies. (greater than 90% of the energy is emitted at in the far-IR). Large luminosity has both starburst and accretion components.
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Beyer, Andrew D., Runyan, M. C., Kenyon, M., Echternach, P. M ., Chui, T., Bumble, B., Bradford, C. M., Holmes, W. A., Bock, J. J.. 2012-06-14. Achieving BLISS: Challenges for Building Fast, Ultra-Sensitive Transition-Edge Sensors. https://ntrs.nasa.gov/citations/20130000256
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