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Realtime Astroparticle Physics

4–6 Feb 2013
Universität Bonn
Europe/Berlin timezone

Contribution List

23 out of 23 displayed
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  1. 7. Welcome and meeting objectives
    Marek Kowalski (University Bonn)
    04/02/2013, 11:10
  2. 8. Gravitational Waves and Multimessenger Astrophysics: high-energy neutrinos and electromagnetic counterparts
    Imre Bartos
    04/02/2013, 11:45
  3. 1. IceCube GRB searches - Toward a realtime search system
    Erik Blaufuss
    04/02/2013, 14:00
    IceCube GRB searches - Toward a realtime search system
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  4. 20. IceCube optical follow-up
    Markus Voge
    04/02/2013, 14:35
  5. 3. Follow-up of the Antares neutrino alerts
    Damien Dornic (CPPM/IN2P3/CNRS)
    04/02/2013, 15:00
  6. 11. The Era of Realtime Astrophysics - The Role of Autonomous Robotic Telescopes
    Carole Mundell
    04/02/2013, 16:00
  7. 12. Fermi, GROND & GRBs
    Arne Rau
    04/02/2013, 16:35
  8. 4. Radio transient searches
    Evan Keane
    04/02/2013, 17:10
    I will review the various methods that have been used in the search for transient radio signals. After introducing the so-called "transient phase space", I will present the highlights of the discoveries from the past few years. Then, I shall focus on a number of as-yet-unexplained signals which might prove to be powerful cosmological probes. Next, I will review the known sources...
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  9. 6. Radio transients in the High Time Resolution Universe radio survey
    David Champion (MPIfR)
    04/02/2013, 17:40
    We are carrying out the most ambitious and comprehensive all-sky survey for pulsars and transient sources to date. Using new digital filterbank backends this survey will create a digital record of the sky that can be data mined in the future and used to search for relativistic binary and millisecond pulsars, RRATs, and extragalactic radio bursts. Using GPU technology we have developed a...
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  10. 0. The Palomar Transient Factory
    Eran Ofek
    05/02/2013, 09:00
    The Palomar Transient Factory
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  11. 5. FRAM -- The Robotic Telescope in the Pierre Auger Observatory
    Radomir Smida
    05/02/2013, 09:35
    F/(Ph)otometric Robotic Atmospheric Monitor is one of the atmospheric monitoring instruments at the Pierre Auger Observatory in Argentina. FRAM is an optical telescope equipped with CCD cameras and it automatically observes a set of selected standard stars. FRAM observations are used to obtain the wavelength dependence of the light extinction. FRAM telescope is also able to observe secondary...
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  12. 2. Gamma-ray Observations of Pulsars with the Fermi LAT
    Lucas Guillemot
    05/02/2013, 10:00
    The Large Area Telescope (LAT) on the Fermi satellite has opened a new era in the study of pulsars, by increasing the population of known gamma-ray pulsars from fewer than 10 to more than 120 objects, thereby establishing pulsars as the dominant class of GeV sources in the Galaxy. The improved sensitivity of the LAT has allowed studies of the light curves and spectra of gamma-ray pulsars with...
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  13. 18. GRB and AGN flare observations with MAGIC
    Josefa Becerra-Gonzalez (University of Hamburg & Instituto de Astrofísica de Canarias (IAC))
    05/02/2013, 11:00
  14. 16. Revealing deaths of massive stars with high-energy neutrinos
    Kohta Murase
    05/02/2013, 11:45
    Neutrinos play important roles in revealing mechanisms of energetic astrophysical explosions such as gamma-ray bursts (GRBs) and supernovae (SNe). The large neutrino detector, IceCube has opened a new window of the multi-messenger astronomy. I overview theoretical prospects of high-energy higneutrino emissions from gamma-ray bursts, newly-born magnetars and luminous supernovae in view of...
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  15. 17. Predictions for Neutrino and Gravitational-Wave Signals of a Future Galactic Supernova
    Thomas Janka
    05/02/2013, 14:00
  16. 9. Ground-based gravitational wave detectors and their capabilities through 2020
    Bruce Allen
    05/02/2013, 14:45
    In this talk I describe the advanced ground-based gravitational-wave detector projects (LIGO in the USA, VIRGO in Italy, GEO in Germany, KAGRA in Japan, LIGO in India), review their status and capabilities, and outline the different signal analysis methods and pipelines that are used. We expect that the first direct detections of gravitational waves (perhaps around 2017) will be from the...
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  17. 10. Gravitational Wave detection using Pulsar networks
    Michael Kramer
    05/02/2013, 16:00
  18. 14. The detection rate of merging neutron stars / black holes
    Thomas Tauris
    06/02/2013, 09:00
  19. 15. The progenitors of SNe and GRBs
    Sung-Chul Yoon (Argelander-Institut für Astronomie, Uni Bonn)
    06/02/2013, 09:30
  20. 13. SWIFT & Neutrinos
    Andreas Homeier
    06/02/2013, 10:00
  21. 21. Astrophysical Multimessanger Observatory Network (AMON)
    Miles Smith
    06/02/2013, 10:55
  22. 22. Putting it all together: Discussion
    06/02/2013, 11:40
  23. 19. MAGICs hunt for GRBs
    Markus Garczarczyk