'Extra galactic' presentation slideshows

1.3k views • 112 slides

TeV II Particle Astrophysics

TeV II Particle Astrophysics. Summary comments. Outline. Introduction: Cosmic-ray spectrum Multi-messenger astronomy TeV astronomy g -ray astronomy n astronomy Gravitational-wave astronomy New detectors. Extra-galactic component ?. n F( n ) for cosmic rays. Air Showers. DIRECT.

773 views • 55 slides

TeV II Particle Astrophysics

TeV II Particle Astrophysics. Summary comments. Outline. Introduction: Cosmic-ray spectrum Multi-messenger astronomy TeV astronomy g -ray astronomy n astronomy Gravitational-wave astronomy New detectors. Extra-galactic component ?. n F( n ) for cosmic rays. Air Showers. DIRECT.

554 views • 55 slides

Exploring the Extreme Universe with GLAST

546 views • 41 slides

Exploring the Extreme Universe with GLAST

416 views • 41 slides

Planck

Planck. Report on the status of the mission Carlo Baccigalupi , SISSA. Outline. CMB The Planck satellite Data processing center Expectations from Planck Planck data. CMB. CMB angular power spectrum. Angle ? 200/ l degrees. CMB angular power spectrum. Acoustic oscillations.

409 views • 39 slides

WMAP 2003

339 views • 33 slides

The cosmic-ray spectrum

454 views • 30 slides

Using the ? -ray Background as a Path to Mapping Dark Matter Clustering in the Universe

Using the ? -ray Background as a Path to Mapping Dark Matter Clustering in the Universe. Eiichiro Komatsu University of Texas at Austin PPC07@Texas A&M, May 18, 2007. K. Ahn & EK, PRD, 71, 021303R (2005); 72, 061301R (2005) S. Ando & EK, PRD, 73, 023521 (2006)

342 views • 26 slides

Using the ? -ray Background as a Path to Mapping Dark Matter Clustering in the Universe

Using the ? -ray Background as a Path to Mapping Dark Matter Clustering in the Universe. Eiichiro Komatsu University of Texas at Austin PPC07@Texas A&M, May 18, 2007. K. Ahn & EK, PRD, 71, 021303R (2005); 72, 061301R (2005) S. Ando & EK, PRD, 73, 023521 (2006)

265 views • 26 slides

Additional Neutrino(s) and CMB Damping Tail

Additional Neutrino(s) and CMB Damping Tail. The timeline of the Universe. Inflation. BBN. recombination. accelerated expansion. reionization. structure formation. Legend of ? CDM. adiabatic, nearly scale invariant, power law, Gaussian fluctuations. +. +. flatness.

381 views • 25 slides

Neutrinos from AGN & GRB

294 views • 21 slides

update on O.W.L. project

update on O.W.L. project. for: CROP summer 2002 by: Dwight Johns RONCALLI date: August 6, 2002. O.W.L. meaning. O rbiting W ide-angle L ight-collectors

237 views • 13 slides

165 views • 7 slides