'Red sequence' presentation slideshows

Clusters as Laboratories for the Study of Galaxy Evolution

1.04k views • 84 slides

Clusters as Laboratories for the Study of Galaxy Evolution

851 views • 84 slides

Science Achievements of the DEEP2/AEGIS survey by S. M. Faber and the DEEP & AEGIS Teams

Science Achievements of the DEEP2/AEGIS survey by S. M. Faber and the DEEP & AEGIS Teams. Supported by CARA, UCO/Lick Observatory, the National Science Foundation, and NASA. DEEP2 basics. Officially finished: ? 53,000 spectra ? 39,000 with Quality 3 or 4 redshifts ? Reliability > 98%.

430 views • 30 slides

Red-Sequence Galaxies with young stars and dust

Red-Sequence Galaxies with young stars and dust. The cluster A901/902 seen with COMBO-17 Christian Wolf (Oxford) Meghan E. Gray (Nottingham) Klaus Meisenheimer (Heidelberg) A&A, in press. A901a. A901a. A901b. A901b. A902. A902. Testing ground: the A901/902 supercluster.

353 views • 30 slides

Red-Sequence Galaxies with young stars and dust

Red-Sequence Galaxies with young stars and dust. The cluster A901/902 seen with COMBO-17 Christian Wolf (Oxford) Meghan E. Gray (Nottingham) Klaus Meisenheimer (Heidelberg) A&A, in press. A901a. A901a. A901b. A901b. A902. A902. Testing ground: the A901/902 supercluster.

306 views • 30 slides

The E SO Dis tant C luster S urvey

357 views • 27 slides

Galaxy in Real Life and Simulations (Leiden, 17/09/2008)

Galaxy in Real Life and Simulations (Leiden, 17/09/2008). When and Where Did Early-Type Galaxies Form?.

326 views • 24 slides

On the formation time scale of massive cluster ellipticals based on deep near-IR spectroscopy at z~2 Masayuki Tanaka (NAOJ) Sune Toft (DARK), Alexis Finoguenov (Helsinki), Mohammad Mirkazemi (MPE), Dave Wilman (MPE), John Mulchaey (Carnegie),

313 views • 22 slides

Max Planck Gesellschaft/ESO 2.2m telescope at La Silla, Chile

366 views • 22 slides

Stellar population results from NFPS: Age and Metallicity along the Red Sequence

Stellar population results from NFPS: Age and Metallicity along the Red Sequence.

270 views • 21 slides

Stellar population results from NFPS: Age and Metallicity along the Red Sequence

Stellar population results from NFPS: Age and Metallicity along the Red Sequence.

259 views • 21 slides

Galaxies and their Environments

Galaxies and their Environments. Nick Cowan UW Astronomy January 26, 2007. Reasonable Questions. Why care about environments? What is an environment? How do we determine environments? How exactly do environments effect galaxies?. Galaxy Environments.

368 views • 20 slides

The Star Formation Histories of Red Sequence Galaxies Mike Hudson U. Waterloo / IAP

The Star Formation Histories of Red Sequence Galaxies Mike Hudson U. Waterloo / IAP Steve Allanson (Waterloo) Allanson, MH et al 09, ApJ 702, 1275 Russell Smith (Durham) Coma/Hectospec team, esp. Ron Marzke. 70% of the stellar mass density is in present red-sequence galaxies

208 views • 20 slides

Evolution of Galaxy Properties from High Redshift to Today

Evolution of Galaxy Properties from High Redshift to Today. AGNs: Where do they live?. Kauffmann et al 2003. In M*>10 10 M ? . Morphologically similar to early-types. OTOH, recent SF similar to late-types (esp. in strong AGN). Kauffmann et al 2004. AGNs and the red sequence.

463 views • 19 slides

Galaxy Populations in the Most Distant Clusters

194 views • 19 slides

Large-scale Structure Simulations

Large-scale Structure Simulations. A.E. Evrard, R Stanek, B Nord (Michigan) E. Gaztanaga, P Fosalba, M. Manera (Barcelona) A. Kravtsov (Chicago) P.M Ricker (UIUC/NCSA) R. Wechsler (Stanford) D. Weinberg (OSU). core science areas. non-linear evolution of the matter density

315 views • 18 slides

What color is the Milky Way?

Jeffrey Newman and Timothy Licquia University of Pittsburgh/Pitt-PACC (Pittsburgh Particle physics, Astrophysics and Cosmology Center). What color is the Milky Way?. janewman@pitt.edu (412) 592-3853 tcl15@pitt.edu (810) 240-9729.

270 views • 14 slides

The scatter and evolution of the color-magnitude relation of elliptical galaxies

154 views • 14 slides

Large Scale Structure at High Redshift in the GOODS Field

Large Scale Structure at High Redshift in the GOODS Field D. Trevese (1), M. Castellano(1), S. Salimbeni (2), A. Grazian (2), L. Pentericci (2), A. Fontana (2), E. Giallongo (2), P. Santini (2), S. Cristiani (3), M. Nonino (3) and E. Vanzella (3)

82 views • 1 slides

CONCLUSIONS:

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

89 views • 1 slides