'Galaxy clusters' diaporamas de présentation

DO NOW

DO NOW. V: 0. Organelle Tissue organ system Organism Population Organ. DO NOW. V: 0. Homework & Agenda. V: 0. TEKS. V: 0. Vocabulary. V: 0. Cells Tissues Organs Organ Systems Organisms Organelles Cell membrane Cell wall Nucleus Cytoplasm Mitochondrion Chloroplast

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THE DARK SIDE

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Ch. 30 Sec. 2

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LOFAR & Particle acceleration in Galaxy Clusters

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Dark Matter and Dark Energy

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Galaxies

Galaxies. Background. Billions of them in the universe Only largest telescopes can gather the light that travels from them to Earth Hubble Deep Field Relatively nearby galaxies 10 billion LY away. Discovery. William Parsons 1845 built a telescope 72 in. diameter

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Dark Energy Survey (DES) Motivation

Dark Energy Survey (DES) Motivation. Dark Energy is the dominant constituent of the Universe Dark Matter is next 95% of the Universe is in Dark Energy and Dark matter for which we have no understanding. 1998 and 2003 Science breakthroughs of the year.

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Observational Evidence of Creation

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MA4: HIGH-ENERGY ASTROPHYSICS

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MA4: HIGH-ENERGY ASTROPHYSICS

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We Discover the Galaxies

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Our Universe Structure

Our Universe Structure. Smallest to largest: Planets ? Stars /Solar systems ?Galaxies?Galaxy Clusters?Universe Universe contains hundreds of billions of galaxies. Galaxies contain hundreds of billions of stars. Imagine the possibility of finding life. Life on other planets IS possible!

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Dark Matter and Dark Energy from the solution of the strong CP problem

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Cosmology with Cluster Surveys

Cosmology with Cluster Surveys. Subha Majumdar Canadian Institute of Theoretical Astrophysics Toronto. along with Joe Mohr, Martin White & Jose Diego. International Conference on Gravitation and Cosmology, Kochi, 5th January 2004. Overview. Introduction to Galaxy Clusters

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GUBBINS

GUBBINS: A novel millimeter-wave heterodyne interferometer. GUBBINS. Paul Grimes Matthew Brock Christian Holler Jaya John Mike Jones Oliver King Jamie Leech Angela Taylor Ghassan Yassin Karl Jacobs Chris Groppi Andrew Harris. Aims:- Prototype mm-wave heterodyne interferometer

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X-ray Optical microwave

X-ray Optical microwave. Cosmology at KIPAC. Dark Energy Survey (DES). The Survey 5000 square degrees (overlap with SPT and VISTA) Five-band (grizY) + VISTA (JHK) photometry to z = 1.5

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The GMRT Radio Halo survey Results and implications for LOFAR

The GMRT Radio Halo survey Results and implications for LOFAR. Simona Giacintucci Harvard-Smithsonian CfA, Cambridge, USA INAF-IRA, Bologna, Italy. T. Venturi, R. Cassano, G. Brunetti, D. Dallacasa, G. Setti (INAF-IRA, Bologna) S. Bardelli (OAB, Bologna).

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Constraining The Distance-Redshift Relation Through Strong Gravitational Lensing of the CMB

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Science Drivers for the Next Generation VHE Telescope(s?)

Science Drivers for the Next Generation VHE Telescope(s?). G. Sinnis with much help from C. Dermer, J. Buckley, H. Krawczynski, S. LeBohec, R. Ong, M. Pohl, S. Swordy, D. Williams, T.C. Weekes. Some History. 2/91, T.C. Weekes, Texas Conference Crab Nebula was the only credible source

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Finding Galaxy Clusters In South Pole Telescope Data

Finding Galaxy Clusters In South Pole Telescope Data. Craig Lawrie Advisor: Dr. John Ruhl. Department of Physics, CWRU. Abstract

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