'Stellar masses' diaporamas de présentation

What shapes galaxy SEDs?

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Sub-mm surveys & galaxy formation SHADES SCUBA2 Jim Dunlop University of Edinburgh

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Chapter 17 Measuring the Stars

Chapter 17 Measuring the Stars. Units of Chapter 17. 17.1 The Solar Neighborhood Naming the Stars 17.2 Luminosity and Apparent Brightness 17.3 Stellar Temperatures More on the Magnitude Scale 17.4 Stellar Sizes Estimating Stellar Radii

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Ingrid Stairs UBC GWPAW Milwaukee Jan. 29, 2011

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SPITZER/IRAC OBSERVATIONS OF GALAXIES AT Z > 2

SPITZER/IRAC OBSERVATIONS OF GALAXIES AT Z > 2. Giovanni G. Fazio Jiasheng Huang Harvard-Smithsonian Center for Astrophysics Cambaridge, MA 02138, USA. IRAC EXTRAGALACTIC GTO PROGRAMS.

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Galaxy Buildup in the First 2 Gyr: The Evolution of the UV LF from z~8 to z~4

Galaxy Buildup in the First 2 Gyr: The Evolution of the UV LF from z~8 to z~4. Rychard Bouwens (University of California, Santa Cruz) Garth Illingworth. August 29, 2007 Venice, Italy Century of Cosmology: Past, Present, Future. N. HST UDF. Galaxy Buildup in the First 2 Gyr.

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Ultraviolet and far-infrared observations of galaxies: constraints on dust attenuation

Ultraviolet and far-infrared observations of galaxies: constraints on dust attenuation. V. Buat, J. Iglesias-Paramo, D. Burgarella, A. Inoue, P. Panuzzo, T. Takeuchi Tracing dust in spiral galaxies:radiative transfer studies in the dawn of a new generation of observing facilities-

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Lecture 9

Lecture 9. 6/18/07 Astro 1001. The Sun. The explanation of how the Sun is giving the Earth so much energy from 150 million kilometers away is very tricky Chemical burning, gravitational contraction not possible Nuclear Fusion is the answer Sun turns mass into thermal energy

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Astrophysics I (8025) Intro. Astrophysics I (4025) A Survey of Astrophysics

Astrophysics I (8025) Intro. Astrophysics I (4025) A Survey of Astrophysics ( excluding planetary). Stellar Brightnesses and Surface Temperatures. Blackbody Radiation. So h? max ? 2.82 kT or. Doing the same in wavelength units:. Stellar Sizes.

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Astrophysics II (822) Intro. Astrophysics II (522) Stellar Astrophysics

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New Views of Galaxies at z~2-3

New Views of Galaxies at z~2-3. Alice Shapley (Princeton) December 12th, 2005. Overview and Motivation. Explosion of z~1.5-3.0 surveys (t lb ~9-11 Gyr)

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Stellar angular momentum evolution in the COROT Mission

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SED measurements of radio galaxies 1 < z < 5

SED measurements of radio galaxies 1 < z < 5. Bob Fosbury (ST-ECF) on behalf of the SHzRGS team Daniel Stern - PI, Peter Eisenhardt (JPL) Carlos De Breuck - Co-PI, Joel Vernet, Alessandro Rettura (ESO) Bob Fosbury (ST-ECF) Andrew Zirm (STSCI) Brigitte Rocca-Volmerange (IAP)

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Testing coherent code for coalescing binaries network analysis

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CONCLUSIONS:

The Cosmic Evolution Survey (COSMOS): galaxy morphologies and colors as a function of mass and environment at z=0.7

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