Universitaet Heidelberg

IAU Beijing 2012

Die Internationale Astronomische Union, abgekürzt IAU, ist eine 1919 gegründete weltweite Vereinigung von Astronomen mit Sitz in Paris. Ihr Ziel ist die Förderung der Astronomie durch internationale Zusammenarbeit.

Die nicht-staatliche Organisation richtet seit 1922 in abwechselnden Ländern alle drei Jahre eine Generalversammlung aus.

Das nächste Treffen findet in Peking am 20.-31. August 2012 statt.

Offizielle Website der IAU Beijing 2012

Sprecher:

Prof. Zhen Cao / China: Gamma-ray astrophysics at the highest energies: the LHASSO project
Prof. Catherine Cesarsky / France: Evolution of gamma-ray astronomy
Prof. John Pretz / USA: Gamma-ray astrophysics at the highest energies: the super-HAWC project
Prof. Tadayasu Dotani / Japan: The multi-wavelength context: X-ray
Prof. Dainis Dravins / Sweden: Extremely high angular resolution optical astronomy
Prof. Anne Green / Australia: The multi-wavelength context: radio
Prof. Jim Hinton / UK: Results of current-generation Cherenkov telescopes
Prof. Werner Hofmann / Germany: Introducing the Cherenkov Telescope Array
Prof. Peter Michelson / USA: Results of current-generation GeV telescopes
Prof. Prof. Subir Sarkar / UK: Dark Energy, Dark Matter, Cosmology relations with the highest energy Universe
Dr. Francesco Massaro / USA: A WISE view of the gamma-ray sky
Dr. Giovanna Pedaletti / Spain: An outlook on PWN and SNRs studies with CTA
Prof. Heino Falcke / Netherlands: LOFAR in the era of CTA
Dr. Christoph Pfrommer / Canada: The Cosmological Impact of TeV Blazars: from Plasma Instabilities to Structure Formation
Dr. Meng Su / USA: Fermi Gamma-ray Bubbles and their possible detection in TeV
Prof. Stefan Wagner / Germany: The highest energy gamma-rays from jets

Programm

JD1: The Highest-Energy Gamma-Ray Universe Observed with Cerenkov Telescope Arrays Program


  • Montag 20. August


Chair: Prof. Anne Green
10:25 – 10:30 Introduction - C. Cesarsky, D. Torres, S. Wagner
10:30 – 11:00 Current-generation GeV telescopes - P. Michelson
11:00 – 11:30 Current-generation Cherenkov telescopes - J. Hinton
11:30 – 12:00 Introducing the Cherenkov Telescope Array, - W. Hofmann
12:00 – 12:30 Gamma-ray astrophysics at the highest energies: the LHASSO project - Z. Cao
Chair: Prof. Zhen Cao
14:00 – 14:30 Gamma-ray astrophysics at the highest energies (HAWC and beyond) - J. Pretz
Astronomy with the future generation of gamma-ray instruments:
14:30 – 15:00 The Highest energy gamma-rays from Jets - S. Wagner
15:00 – 15:30 Fermi Gamma-ray Bubbles and their possible detection in TeV, MPEG - Meng Su
Chair: Prof. Peter Michelson
16:00 – 16:30 Dark Energy / Dark Matter / Cosmology - S. Sarkar
16:30 – 17:00 Extremely high angular resolution optical astronomy with Cherenkov telescopes - D. Dravins
17:00 – 17:30 The multi-wavelength context of the future gamma-ray instruments: X-rays - T. Dotani
17:30 – 18:00 The Cosmological Impact of TeV Blazars: from Plasma Instabilities to Structure Formation - Christoph Pfrommer

  • Dienstag 21. August
Chair: Prof. Werner Hofmann
10:30 – 11:00 The multi-wavelength context of the future gamma-ray instruments: radio, MPEG - A. Green
11:00 – 11:20 LOFAR in the era of CTA, MPEG1, MPEG2, MPEG3 - Heino Falcke
11:20 – 11:40 An outlook on PWN and SNRs studies with CTA - Giovanna Pedaletti
11:40 – 12:00 A WISE view of the gamma-ray sky - Francesco Massaro
12:00 – 12:30 Evolution of gamma-ray astronomy - C. Cesarsky


Wissenschaftlicher Ausschuss:


Aya Bamba (Japan & Ireland)
Zhen Cao (China)
Catherine Cesarsky (France, SOC-Chair)
Dainis Dravins (Sweden)
Brenda Dingus (USA)
Tadayasu Dotani (Japan)
Luke Drury (Ireland)
Anne Green (Australia)
Felix Mirabel (Argentina & France)
Helene Sol (France)
Diego F. Torres (Spain, JD-IAU Contact)
Meg Urry (USA)
Stefan Wagner (Germany, SOC-Chair)
Shuang-Nan Zhang (China)
to top of page