'1 mpc' presentation slideshows

AY202a Galaxies & Dynamics Lecture 16: Galaxy Groups & Clusters

AY202a Galaxies & Dynamics Lecture 16: Galaxy Groups & Clusters. Galaxies Are Not Randomly Distributed in Space. Fundamental discovery (and debate) in the 20th century is that Galaxies cluster. On small scales: Binaries ~100 kpc

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Luigina Feretti Istituto di Radioastronomia CNR Bologna, Italy

Radio observations of cluster mergers. Luigina Feretti Istituto di Radioastronomia CNR Bologna, Italy. X-Ray and Radio Connections, Santa Fe, NM February 3-6, 2004. OUTLINE. Diffuse cluster radio emission: radio halos and relics ? non-thermal components of the ICM

587 views • 46 slides

Bright Side versus Dark Side of Star Formation: UV and IR Views

Bright Side versus Dark Side of Star Formation: UV and IR Views. C. Kevin Xu, IPAC, Caltech Veronique Buat, LAM, Marseille. Collaborators: J. Iglesias-Paramo, T. Tekeuchi, M. Rowan-Robinson, GALEX team, SWIRE team.

588 views • 44 slides

5A-3 Astrophysics Cosmology

5A-3 Astrophysics Cosmology. Astrophysics booklet pages 54 to 65. August 21st, 2010. AQA A2 Specification. The Doppler Effect. As the ambulance travels forwards: The sound wave in front is compressed - decreasing its wavelength - increasing its frequency

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546 views • 43 slides

Large Scale Structure of the Universe at high redshifts

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Cosmic Voids and Void Galaxies

Cosmic Voids and Void Galaxies. Michael S. Vogeley Department of Physics Drexel University vogeley@drexel.edu. KIAS Workshop , October 27-28, 2008. SDSS galaxy map. Voids as Cosmic Laboratories. Voids form by gravity through expansion of initially underdense regions

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E ? L

510 views • 37 slides

The Filament-Void Network and the Scale of Homogeneity in the Universe

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Cosmological N-Body Simulation - Topology of Large scale Structure

Cosmological N-Body Simulation - Topology of Large scale Structure. CCP 2006. 8. 29. Changbom Park with Juhan Kim (Korea Institute for Advanced Study) & J. R. Gott (Princeton) , J. Dubinski (CITA). History of Universe. Theme: Origin & Formation Mechanism of Cosmic Structures.

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454 views • 30 slides

Topology of Large Scale Structures Introduction, Theory and Progress Report

440 views • 29 slides

Large Scale Structure of the Universe at high redshifts

462 views • 28 slides

The Warm-hot Gaseous Halo of the Milky Way

The Warm-hot Gaseous Halo of the Milky Way. Smita Mathur The Ohio State University With Anjali Gupta, Yair Krongold, Fabrizio Nicastro, M. Galeazzi. In the low-redshift Universe, baryons are missing on all scales. Galaxies. Universe. Clusters. Where are the Galactic missing baryons?.

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AGGREGATE EXPENDITURES

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Takuya Akahori Chungnam National University

Exploring Faraday Rotation Measure due to the Intergalactic Magnetic Field with the Square Kilometer Array. Takuya Akahori Chungnam National University. Contents. Introduction Faraday Rotation Measure (RM) due to the Intergalactic Magnetic Field (IGMF) Part 1. present-day local universe

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Using Symmetry to Detect Velocities with kinetic SZ

Using Symmetry to Detect Velocities with kinetic SZ. “The combination of CMB and LSS is more than the sum of it’s parts”. Albert Stebbins Fermilab. External Correlations of the CMBR & Cosmology Fermilab, Batavia 25-26 May 2006. Why Velocities?.

221 views • 11 slides

Virtual Observatory & HORIZON project

Virtual Observatory & HORIZON project. H. Wozniak 1 , and HORIZON 2 consortium 1 CRAL 2 CEA/SAp, CRAL, IAP, LERMA, LUTH. Horizon project: computational astrophysics on massively parallel systems to understand formation and evolution of structure and galaxies in the universe.

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The Multiplier

The Multiplier. Multiplier. You may recall the RGDP by the expenditure approach is made up of the real levels of C, I, G and Xn in the following way: RDGP = C + I + G + Xn.

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Status of the S5 calibration

Status of the S5 calibration. Michael Landry For the Calibration Committee LSC September 2008. Outline. h(f) Status V3 summary. V4 status - improvements. Expectations for S6 calibration. Next talk: Xavier Siemens: h(t) report V3 h(t) - validation, systematics, hardware injections. S6.

254 views • 10 slides