PPT-SPIE 7734, Optical and Infrared Interferometry II, San Diego, June 2010

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Dainis Dravins Hannes Jensen Lund Observatory Sweden Stephan LeBohec Paul D Nuñez The University of Utah Salt Lake City STELLAR INTENSITY INTERFEROMETRY Astrophysical

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SPIE 7734, Optical and Infrared Interferometry II, San Diego, June 2010: Transcript


Dainis Dravins Hannes Jensen Lund Observatory Sweden Stephan LeBohec Paul D Nuñez The University of Utah Salt Lake City STELLAR INTENSITY INTERFEROMETRY Astrophysical targets for sub. Proc. of SPIE Vol. 7657 76570K-2 Proc. of SPIE Vol. 7657 76570K-3 Proc. of SPIE Vol. 7657 76570K-4 Proc. of SPIE Vol. 7657 76570K-5 Proc. of SPIE Vol. 7657 76570K-6 Proc. of SPIE Vol. 7657 76570 (with a digression on reference pixels). Bernard J. Rauscher. NASA Goddard Space Flight Center. 22 July 2010. 1. STScI Calibration Workshop. JWST NIRSpec HAWAII-2RG. Introduction. After the diameter of the primary mirror, no component affects the performance of an observatory more than the detectors. limits on . dark . energy. Jun. 17. 2011. Geena Kim. P. Hamilton, D. Schlippe, and H. Mueller. University of California, Berkeley. Paul Hamilton. Müller group. University of California at Berkeley. . 1. Les gens ont des . étoiles qui ne sont pas les mêmes.. Pour les uns qui voyagent, elles sont des guides.. Pour les autres, elles ne sont rien que des petites lumières.. Pour d’autres, qui sont savants, elles sont des problèmes.. 11/5/2014. T-Dwarfs. Artist's vision of a T-dwarf. M dwarf. L dwarf. T dwarf. Jupiter. ~1600 K. ~650 K. 160 K. ~2800 K. INTRODUCTION. T dwarfs. . are a class of low mass, low . temperature(600 –1300 . polarised. emission in X-ray binaries. Dave Russell. New York University Abu Dhabi. dave.russell@nyu.edu. In collaboration with T. ariq . Shahbaz. (IAC, Tenerife). I’d also like to thank Rob Fender, Elena Gallo, . 14. CO. 2. ) at and below ambient levels. D. A. Long, . A. J. Fleisher, Q. Liu, and J. T. Hodges. National Institute of Standards and Technology. Gaithersburg, Maryland. HDR Architecture, Inc.. Long-lived isotope of carbon (half-life 5,730 years). | Slide . 1. A Very Brief Introduction to Infrared Spectroscopy. © ABB Group . June 19, 2014. | Slide . 2. Basics of the Technique. © ABB Group . June 19, 2014. | Slide . 3. Infrared Spectroscopy. Properties of III-Nitride . H. eterostructures. Oana . Malis, Purdue University. EPM DMR 1206919. The principal objective of this project . is . to establish the relationship between material growth, atomic structure and infrared optical properties of nitride semiconductors. A. A Tutorial on Optomechanical Tolerancing and a Synopsis of the Economics Involved. Ezra Milby . OPTI 521 – Optomechanical Engineering. Fall 2009 – Prof. J.H. Burge. 30 November 2009. E. Milby - OPTI521 - Intro to Optomech Eng. | Slide . 1. A Very Brief Introduction to Infrared Spectroscopy. © ABB Group . June 19, 2014. | Slide . 2. Basics of the Technique. © ABB Group . June 19, 2014. | Slide . 3. Infrared Spectroscopy. Britton Chance: . Life, Times, & Legacy . Symposium and Workshop. Translational . Research in. Near Infrared Based Functional Brain Imaging. Banu . Onaral, PhD. H.H. Sun Professor and Director. School of Biomedical Engineering, . Optical interferometry is a powerful technique to make images on angular scales hundreds of times smaller than is possible with the largest telescopes. This concise guide provides an introduction to the technique for graduate students and researchers who want to make interferometric observations and acts as a reference for technologists building new instruments. Starting from the principles of interference, the author covers the core concepts of interferometry, showing how the effects of the Earth\'s atmosphere can be overcome using closure phase, and the complete process of making an observation, from planning to image reconstruction. This rigorous approach emphasizes the use of rules-of-thumb for important parameters such as the signal-to-noise ratios, requirements for sampling the Fourier plane and predicting image quality. The handbook is supported by web resources, including the Python source code used to make many of the graphs, as well as an interferometry simulation framework, available at www.cambridge.org/9781107042179. Achuta . Kadambi. , Jamie . Schiel. and Ramesh . Raskar. , IEEE CVPR16 . An interferometric 3D camera for multipath imaging for meter scale scenes. Swept Frequency Electronic Interferometry. Take-home message:.

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