'Rest frame' diaporamas de présentation

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spectroscopic diversity of SNe Ia in the near-infrared

Eric Y. Hsiao University of Victoria. spectroscopic diversity of SNe Ia in the near-infrared. SNe Ia in the near-infrared why?. less dust extinction low redshift standard candles in JHK bands independent measure of Hubble constant high redshift rest frame I band Hubble diagram

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Massive Galaxies at high redshift

Massive Galaxies at high redshift. GOODS http://www.stsci.edu/science/goods Lewnida s (Lexi) Moustakas Space Telescope Science Institute M Dickinson, H Ferguson, M Giavalisco R Somerville, T Dahlen, B Mobasher, H Yan. ~3x10 10 M o. The SDSS z~0 age/stellar mass relation. age.

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SFR and COSMOS

SFR and COSMOS. Bahram Mobasher + the COSMOS Team. COSMOS offers:. Extensive multi-waveband surveys from radio to X-ray Large area coverage ( 2 sq. deg.) HST/ACS morphologies (B/D, Sersic, concentration, asymmetry, clumpiness)

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Electricity and Magnetism II

12 .1. Electricity and Magnetism II. Griffiths Chapter 12 Relativity Clicker Questions. Two major results of special relativity are Time Dilation and Lorentz Contraction. Please pick one of the choices below which best describes how well you feel you understand them. 12 .2.

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The size evolution of early-type galaxies since z=2

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General Relativity Physics Honours 2009

General Relativity Physics Honours 2009. Florian Girelli Rm 364, A28 girelli@physics.usyd.edu.au Lecture Notes 5. Courses on the 16 th September are cancelled due to a university strike. Instead they will be on the 23 rd September, from 10am to 12pm

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Modern Quasar SEDs

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Images of quark intrinsic motion in covariant parton model

Images of quark intrinsic motion in covariant parton model. P etr Za vada Inst itute of Physics, Prague , Czech Republic. ( based on collaboration and discussions with A.Efremov , P.Schweitzer and O.Teryaev ). Outline. 3D covariant parton model general remarks

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Determination of the J PC of the X(3872) (Reviews of BN800)

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Lightcones for Munich Galaxies

Lightcones for Munich Galaxies. Bruno Henriques. Outline. 1. Model to data - stellar populations and photometry. 2. Model to data - from snapshots to lightcones. 3. Results - pencil beams. 4. Results - all-sky cones. Mass to Light. Stellar Population Synthesis. Metallicity + Age +IMF.

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Flavor Structure of the Nucleon Sea from Lattice QCD

Flavor Structure of the Nucleon Sea from Lattice QCD. Jiunn-Wei Chen National Taiwan U. Collaborators: Huey-Wen Lin, Saul D. Cohen, Xiangdong Ji arXiv: 1402.1462. Lattice PDF: from Moments to the Sea. Quark PDF in a proton:

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PHYS 221 Recitation

PHYS 221 Recitation. Kevin Ralphs Week 12. Overview. HW Questions Chapter 27: Relativity History of Special Relativity (SR) Postulates of SR Time Dilation Simultaneity Length Contraction Velocity Addition Mass, Energy and Momentum. History of SR.

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Molecular Dynamics Simulation of Longitudinal Space-Charge Induced Optical Microbunching

Molecular Dynamics Simulation of Longitudinal Space-Charge Induced Optical Microbunching. A. Marinelli, J. B. Rosenzweig and A. Pham UCLA Dept. of Physics and Astronomy FEL 2009, Liverpool, UK August 25, 2009. The Problem.

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Black hole accretion and host galaxies of obscured quasars

Black hole accretion and host galaxies of obscured quasars. Vincenzo Mainieri . with. Angela Bongiorno, Andrea Merloni & COSMOS. Introduction. AGN-galaxies co-evolution.

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Nicholas Bond (Rutgers University)

Stellar Populations of High-Redshift Star-Forming Galaxies Using Rest-Frame Optical and UV Imaging. Nicholas Bond (Rutgers University) Collaborators: Eric Gawiser (Rutgers), Caryl Gronwall (PSU), Robin Ciardullo (PSU), John Feldmeier (YSU), Ana Matkovic (PSU)

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Neutral Kaons and CP violation

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