PPT-Optical/Infrared Astronomy of AST3

Lifan Wang TAMUCCAA The Site Dome A Elevation 4091 m 13422 ft Coordinates 80d22m E77d 21m The highest peak on the Plateau Marching toward Antarctica A team of Pioneers led by Yuanshen. Lee ShihFu Lee Jan M Gildemeister and Paul L Richards Department of Physics University of California Berkeley CA 94720 Center for Particle Astrophysics University of California Berkeley CA 94720 Material Science Division Lawrence Berkeley National Bin Ma, . Peng. Wei, Yi . Hu. , . Zhaohui. Shang. NAOC. 2015.03.10. 2015 AST3 . meeting@HKU. Variables by . Lingzhi. Wang. Outline . 1 Overview of the data . 2 Image Reduction. 3 Astrometry. 4 Aperture Photometry. Julie Cass. SULI Program 2011. SLAC National Accelerator Center. Advisor Josef Frisch. Overview of Spectrometer Optics . 90° . off-axis parabolic mirrors . (OAP) . . HeNe. laser . at 632.816 nm (visible) to align optics. 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 . Science of SOFIA: . NASA’s Airborne Infrared Observatory. Presented by: Kathy Ivey Wilson, Comal ISD. Steven Biles, McKinney ISD. Presentation Outline. TEKS for Activity. Why Airborne Astronomy?. SOFIA program history. 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, . for the AST3-3 telescope for the Kunlun Infrared Sky Survey (KISS). Progress Meeting. Jon Lawrence. 14 August 2015. Project Aims and Objectives. Project Personnel. Project Roles. Jeremy . Mould (SUT) as Lead Investigator. Ma Bin (NAOC). 2015.03.09. 2015 AST3 . meeting@HKU. OUTLINE. 1 AST3 CCD. 2 CCD . test results. 3 Nonlinear PTC. 4 Current status. 1 AST3 CCD. STA 1600FT. 10560 * 10560 pixels. Pixel size 9. μ. m -> 1”. 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). 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-. Astronomy. , derived from the Greek words for . star law. , is the scientific study of all objects beyond our world. . Astronomy is not a “stand-alone” science. . It combines areas from a number of other fields, including mathematics, chemistry, geology, biology and physics. . 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. . Astronomy. , derived from the Greek words for . star law. , is the scientific study of all objects beyond our world. . Astronomy is not a “stand-alone” science. It combines areas from a number of other fields, including mathematics, chemistry, geology, biology and physics. . J . Václavík 1 , D . V ápenka 1 1 Institute of Plasma Physics ASCR v.v.i., TOPTEC, Sobotecká 1660, 51101 Turnov, Czech Republic Abstract. Gallium phosphide is interesting material for optical sy