タイトル | Achieving BLISS: Challenges for Building Fast, Ultra-Sensitive Transition-Edge Sensors |
著者(英) | Beyer, Andrew D.; Bock, J. J.; Bradford, C. M.; Holmes, W. A.; Kenyon, M.; Chui, T.; Echternach, P. M .; Runyan, M. C.; Bumble, B. |
著者所属(英) | Jet Propulsion Lab., California Inst. of Tech. |
発行日 | 2012-06-14 |
言語 | eng |
内容記述 | 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. |
NASA分類 | Astronomy |
権利 | Copyright |
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