PPT-Fermi LAT Observation of Supernova Remnants

Xia Fang Problems Thanks for your time. G & G Floor Covering, you will find that we carry all types of carpeting right here in our warehouse. Most carpet is 12 foot wide and sold by the square yard. From neutral colors and traditional naps to unique size and area rugs, we have it all, including: (Fermi acceleration at shock: most standard, nice powerlaw, few free parameters). main . signatures to . be determined: . E. min . , . E. max. [. Ã. timescale . t. acc. (E. ) ], . spectral slope . 1. John Beacom, The Ohio State University. 2. Plan of the Talk. Introduction to Supernova . N. eutrinos. Focus on . B. urst . D. etection. . What will we know after the next burst?. What . new capabilities do we need?. N. eutron . Stars Foreseen. . Supernova . End Products?. When a . supernova. goes off, we can speculate that:. The star might blow itself to smithereens, . scattering all its material into space and leaving . in Tunnel Junctions. Jin Zhang. , Y. Sherkunov, N. d’Ambrumenil, B. Muzykantskii. University of Warwick, U.K.. APS March Meeting, Portland, 17. th. , March, 2010. Fermi-Edge Singularity. Sudden change . with WFIRST . DRM1 and DRM2. C Baltay. June 1, 2012. Supernova Surveys . using . Slitless. Spectroscopy. Use Imager for . SNe. discovery and to get . lightcurves. Use . slitless. spectroscopy to type supernovae and get redshifts. Instrument Chemistries for each step in the decontamination process. Pre-cleaning. Manual cleaning. Automated cleaning. © 2010 Case Medical, Inc.. Case Solutions. CSR Ink and adhesive remover. SchmutzOff stainless steel, acid based re-conditioner and . Fermi National Accelerator Lab December 13, 2017 . How we usually think of him. Or perhaps . l. ike . t. his . How I think of him. There’s a story behind that orange line on the right of the image…... Fermi LAT Overview Fermi Solar Workshop August 2012 The Large Area Telescope The LAT is a particle physics detector we’ve shot into space We analyze individual events (one photon at a time) with high energy physics techniques to get photon sample USING DATA ON EXTRAGALACTIC DIFFUSE . GAMMA-RAY EMISSION. . A. . Uryson. Lebedev. Physical Institute RAS, . Moscow. INTRODUCTION. UHECR data are obtained by Pierre Auger Observatory (PAO) and Telescope Array (TA):. DPF 2015 – University of Michigan, Ann Arbor. . Alejandro Lopez . in collaboration with: C. Savage, D. Spolyar and D. Adams. Outline:. Brief Introduction. Goal. Technique. Results. Conclusion. Future Work. Francesco Loparco*. Salvatore De Gaetano, Mario Nicola . Mazziotta. . on behalf of the Fermi LAT Collaboration. *e-mail: francesco.loparco@ba.infn.it. The gamma-ray Moon. 1. The Moon is among the brightest sources in the gamma-ray sky. T. elescope. Liz Hays. NASA GSFC. Lecture Plan. The Fermi Observatory. Science Motivation. Instruments. Detecting gamma rays with the Large . A. rea Telescope. Instrument Subsystems. Angular resolution. Semiconductors. Faculty Name : . Dr.Anju. Dixit MSME Department UIET CSJM University Kanpur. 1. Course . Code: MSE-S303 . . Electronic . and Optical Materials. Recap. The material which has electrical conductivity between that of a conductor and that of an insulator is called as semiconductor. Silicon, germanium and graphite are some examples of semiconductors..