'1 mjy' presentation slideshows

History of IGM

History of IGM. ionized. C.Carilli (NRAO) CfA Sept 2004. neutral. Epoch of Reionization (EoR). bench-mark in cosmic structure formation indicating the first luminous structures. ionized. z=5.80. z=5.82. z=5.99. z=6.28. The Gunn Peterson Effect.

632 views • 53 slides

History of IGM

History of IGM. F(HI) = 0. C.Carilli (NRAO) Heidelberg 05. F(HI) = 1. Epoch of Reionization (EoR). last phase of cosmic evolution to be tested bench-mark in cosmic structure formation indicating the first luminous structures. F(HI) = 1e-5. z=5.80. z=5.82. z=5.99. z=6.28.

570 views • 48 slides

391 views • 30 slides

Physics of the Formation and Evolution of Galaxies Report from the High-z Working Group

Physics of the Formation and Evolution of Galaxies Report from the High-z Working Group. Tsutomu T. TAKEUCHI (Nagoya University) Hiroyuki HIRASHITA (ASIAA ) Shuichiro YOKOYAMA (Nagoya University) and members of the high- z working group.

352 views • 25 slides

Spitzer Thermal Radiometry of TNOs

Spitzer Thermal Radiometry of TNOs. John Stansberry Will Grundy John Spencer Mike Brown Dale Cruikshank. Overview. Spitzer TNO projects and sample Multiband Imaging Photometer for Spitzer (MIPS) Characteristics Data processing Data and Results for Particular Objects

349 views • 23 slides

Structure in the sub-mm background towards the HDF

Structure in the sub-mm background towards the HDF. John Peacock & the UK sub-mm survey consortium. Novartis Institute, November 1999. Outline. Motivation for resolving the sub-mm background The SCUBA 850- m m map of the HDF Optical identifications of the S 850 > 2 mJy sources

267 views • 16 slides

Four hot DOGs eaten up with the EVN

243 views • 15 slides

287 views • 14 slides

The Quasar 1317+520: A Laboratory for Particle Acceleration

The Quasar 1317+520: A Laboratory for Particle Acceleration. Svetlana Jorstad IAR, Boston U Alan Marscher IAR , Boston U Jonathan Gelbord U. Durham

250 views • 12 slides

Scientific Interests

Scientific Interests. The nature of active galaxies with redshift: power source, feedback; Probe the energetics and dynamics of the central regions in molecular lines High mass star formation: IMF. Facilities.

121 views • 4 slides