'Redshift' presentation slideshows

1.01k views • 80 slides

Probe of Dark-Energy with Large Scale Structures

Yong-Yeon Keum KPS-2007, Jeju October 18, 2007. From CMB + SN1a + structure formation. Probe of Dark-Energy with Large Scale Structures. Experimental evidences of accelerating universe Candidates of Dark Energy Probe of Dark-Energy with Large Scale Structures Summary. Contents.

772 views • 62 slides

PISCO Progress

756 views • 60 slides

r = 3 H 2 /8 p G

646 views • 51 slides

Spectrum Synthesis and Supernovae

641 views • 47 slides

Orbital Energy and Escape Velocity

891 views • 39 slides

Universe in a box: simulating formation of cosmic structures

Universe in a box: simulating formation of cosmic structures. Andrey Kravtsov Department of Astronomy & Astrophysics Center for Cosmological Physics (CfCP) University of Chicago http://astro.uchicago.edu/~andrey /talks/ http://cfcp.uchicago.edu/lss/. Galaxies. Galaxy Clusters.

511 views • 38 slides

21cmFAST A Fast, Semi-Numerical Simulation of the High-Redshift 21cm Signal

21cmFAST A Fast, Semi-Numerical Simulation of the High-Redshift 21cm Signal. Mesinger, Furlanetto , & Cen (2010). Andrei Mesinger Princeton University. Motivation. We know next to nothing about high-z --> ENORMOUS parameter space to explore

664 views • 29 slides

Eric Linder University of California, Berkeley Lawrence Berkeley National Lab

Course on Dark Energy Cosmology at the Beach 2009. Eric Linder University of California, Berkeley Lawrence Berkeley National Lab. JDEM constraints. Outline. Lecture 1: Dark Energy in Space The panoply of observations Lecture 2: Dark Energy in Theory The garden of models

426 views • 28 slides

The Alcock-Paczynski Probe of Cosmology

The Alcock-Paczynski Probe of Cosmology. Lyman- ? forest, LSS, And Cosmic Consistency. Albert Stebbins Fermilab. Dark Energy Workshop Center for Cosmological Physics University of Chicago 15 December 2001. z. ?.

514 views • 21 slides

The observations of GRB optical afterglow with 6-meter telescope:

The observations of GRB optical afterglow with 6-meter telescope: recent results and future plans T.A. Fatkhullin and SAO RAS follow-up team. Nizhnij Arkhyz, 2009. History of the 6-meter telescope proposal. 10 years (1999-2009) of the GRB observation program (P.I.: A.J. Castro-Tirado)

389 views • 20 slides

AGN

AGN. Jason Jeong. Intro: AGN. AGN stands for active galactic nuclei. It is the core of the galaxy that produces more radiation than the rest of the galaxy. Intro: AGN. It is an active galaxy because of one of the following:

415 views • 19 slides

Photometric Redshifts: Some Considerations for the CTIO Dark Energy Camera Survey

Photometric Redshifts: Some Considerations for the CTIO Dark Energy Camera Survey. Huan Lin Experimental Astrophysics Group Fermilab. Outline. Photometric Redshifts for Red (Cluster) Galaxies Illustration using the SDSS luminous red galaxy (LRG) sample

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268 views • 16 slides

by Fidy A. RAMAMONJISOA MSc Project University of the Western Cape

Modelling radio galaxies in simulations: CMB contaminants and SKA / Meerkat sources. by Fidy A. RAMAMONJISOA MSc Project University of the Western Cape. Supervisor : Prof Catherine Cress. SKA 4 th annual Bursary Conference, Stellenbosch Institute for Advanced Study 03/12/09.

297 views • 14 slides

Evolution of the IGM/Galaxy Halo Interface to z=2

Evolution of the IGM/Galaxy Halo Interface to z=2. Chris Churchill (New Mexico State University) Wal Sargent (Caltech) Michael Rauch (Carnegie). Evolution of the IGM/Galaxy Interface to z=2. Abstract.

288 views • 12 slides

Clusters, Galaxies and the COSMOS

228 views • 11 slides

A relation to estimate the redshift from the X-ray afterglow light curve

157 views • 9 slides

The Big Bang

590 views • 6 slides

CA Collins et al. Nature 458 , 603-606 (2009) doi:10.1038/nature07865

The stellar evolution of BCGs with redshift. CA Collins et al. Nature 458 , 603-606 (2009) doi:10.1038/nature07865.

96 views • 1 slides