'Galaxy properties' presentation slideshows

Chapter 15 Normal and Active Galaxies

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MOS Scientific Applications

MOS Scientific Applications. Michael Balogh University of Durham. MOS Scientific Applications (mostly galaxy clusters). Michael Balogh University of Durham. Outline. Galaxy Clusters: scientific motivation Canadian Network for Observational Cosmology (CNOC)

569 views • 46 slides

The Build-up of the Red Sequence at z<1.3

Masayuki Tanaka ( ESO, not STScI ) + Taddy Kodama (NAOJ). The Build-up of the Red Sequence at z<1.3. galaxies come in two flavours. red. blue. bright. faint. Conclusion.

527 views • 43 slides

Are galaxies still evolving strongly? Christopher J. Miller

The Effects of Environment. Hubble Heritage Image. On Galaxy Evolution at Low-z. Are galaxies still evolving strongly? Christopher J. Miller. Part I. Defining the questions, methods, and tools of the research topic. Physical Processes of Galaxies. Galaxy Interactions.

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Wide-field Imaging + Spectroscopic Survey of Distant Clusters

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Investigating Galaxy Evolution with Empirical Population Synthesis

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How Standard are Cosmological Standard Candles?

How Standard are Cosmological Standard Candles?. Mathew Smith and Collaborators (UCT, ICG, Munich, LCOGT and SDSS-II) SKA Bursary Conference 02/12/2010. Introducing Type Ia Supernova. One of the (optically) brightest astrophysical phenomena, so can be seen to large distances

378 views • 19 slides

The connection between Lyman-alpha absorption in low-redshift quasars and intervening galaxies

The connection between Lyman-alpha absorption in low-redshift quasars and intervening galaxies. Johen Liske. Tutor:. Alizera Aghaee, Begona Ascaso Angles, Ryan Houghton, Yuri Bialetski. What are quasars ?. The first quasar (3C273) was discovered in 1963

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Tracing Dark and Luminous Matter in COSMOS: Key Astrophysics and Practical Restrictions

Tracing Dark and Luminous Matter in COSMOS: Key Astrophysics and Practical Restrictions. COSMOS high-z convergence map Richard Massey. James Taylor (Caltech) -- Cosmos meeting -- Kyoto, Japan -- May 24 -- 2005. Tracing the Matter Distribution with Lensing: Key Astrophysics.

284 views • 16 slides

Spectroscopic Indicators of Galaxy Evolution:

Spectroscopic Indicators of Galaxy Evolution:. Early-type Galaxies in Cl0024+16 at z~0.4. Sean Moran Ge/Ay 132. Large Scale Surveys of Cl0024+17 (z~0.39) and MS0451-03 (Z~0.54). Cl0024: 39 sparsely sampled WFPC2 images, to 5 Mpc Spectra of over 200 members MS0451:

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luminosity & color of galaxies in clusters

luminosity & color of galaxies in clusters. sarah m. hansen university of chicago with erin s. sheldon (nyu) risa h. wechsler (stanford). astrophysics with eV photons. sarah m. hansen university of chicago with erin s. sheldon (nyu) risa h. wechsler (stanford). outline. motivation

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Convergence Bin

Relating Mass and Light in the COSMOS Field J.E. Taylor, R.J. Massey ( California Institute of Technology), J. Rhodes ( Jet Propulsion Laboratory) & the COSMOS Team.

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