'3 mjy' presentation slideshows

ALMA: Resolving (optically) obscured galaxy formation Dusty04, C. Carilli (NRAO)

ALMA: Resolving (optically) obscured galaxy formation Dusty04, C. Carilli (NRAO). IR. Optical. Franceschini 2000. Cosmic Background Radiation. Obscured galaxy formation: low redshift (Meier & Turner 2004). IC342 distance = 2 Mpc M _gas = 4e7 M _sun SFR = 0.1 M _sun /yr

418 views • 32 slides

ALMA: Resolving (optically) obscured galaxy formation Dusty04, C. Carilli (NRAO)

ALMA: Resolving (optically) obscured galaxy formation Dusty04, C. Carilli (NRAO). IR. Optical. Franceschini 2000. Cosmic Background Radiation. Obscured galaxy formation: low redshift (Meier & Turner 2004). IC342 distance = 2 Mpc M _gas = 4e7 M _sun SFR = 0.1 M _sun /yr

403 views • 31 slides

Understand Galaxy Evolution with IR Surveys:

366 views • 26 slides

PAST search for Reionization

PAST search for Reionization. Ue-Li Pen ???. Xiang-Ping Wu ??? , Jeff Peterson. Successes and Limitations in Cosmology. -CMB PS accuracy up to 1% -Cosmological parameters require low z normalization. -error bars on galaxy surveys: on small scales non-linear, stochastic, biased. 10%?

314 views • 25 slides

The Accretion History of SMBHs in Massive Galaxies

The Accretion History of SMBHs in Massive Galaxies. Kate Brand STScI Collaborators: M. Brown, A. Dey, B. Jannuzi, and the XBootes and Bootes MIPS teams. Tucson, November 2006. Questions. How did the mass of SMBHs grow? How is this related to the build-up of the red sequence?

283 views • 19 slides

Mapping the COSMOS at 1 mm using Bolocam

Mapping the COSMOS at 1 mm using Bolocam. James Aguirre University of Colorado, Boulder

173 views • 11 slides

A Sub-mm View of Debris Disks: The case for CCAT exploration

A Sub-mm View of Debris Disks: The case for CCAT exploration. ? Corvi Wyatt et al. (2005). 450 ?m. 850 ?m. Sally Dodson-Robinson University of Texas. Spitzer 160 ?m. HD 207129: 16 pc 152-158 mJy HD 10647: 17 pc 451-462 mJy HD 115617 (not shown): 8.5 pc 89-141 mJy

164 views • 8 slides

High Angular Resolution SMA Imaging of High Redshift Galaxies at 345 GHz

BR1202S. BR1202N. References: Borys, C. et al, 2006, ApJ, 636, 134 Giavalisco,M. et al, 2004, ApJ, 600, L93 Iono, D. et al, 2006, ApJ, 645, L97 Iono, D. et al, 2006, ApJ, 640, L1 Iono, D. et al, 2006b, PASJ, 58, 6 (in press) Jannuzi, B. & Dey, A., 1999, ASP 191, p111

133 views • 1 slides