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Blois 2017: 29th Rencontres de Blois on "Particle Physics and Cosmology"

28 May 2017 to 2 June 2017
Europe/Paris timezone

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Session

Parallel Session Astro+Cosmo

31 May 2017, 14:00

Conveners

Parallel Session Astro+Cosmo

  • Anna Franckowiak (DESY)

Parallel Session Astro+Cosmo

  • Fabian Schmidt (MPA-Garching)

Presentation materials

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  1. 59. ANTARES highlights and KM3NET/ARCA prospects
    Sergio Navas Concha (Universidad de Granada (ES))
    31/05/2017, 14:00
  2. 60. Astrophysical neutrinos at IceCube, a new window to the Cosmos
    Mohamed Rameez (NBI Kopenhagen)
    31/05/2017, 14:20
  3. 45. Results from ARIANNA
    Allan Hallgren (Uppsala University)
    31/05/2017, 14:40
  4. 95. The Very-High-Energy Gamma-ray Sky: Recent Results from VERITAS
    Elisa Pueschel (DESY)
    31/05/2017, 15:00
  5. 48. Results from H.E.S.S.
    Francois Brun (CENBG, Bordeaux)
    31/05/2017, 15:20
  6. 66. Exploring the cosmic middle age with MAGIC
    Dr Giacomo Bonnoli (Università degli Studi di Siena & INFN Pisa)
    31/05/2017, 15:40
  7. 44. The Einstein@Home Gamma-ray Pulsar Survey
    Colin Clark (AEI Potsdam)
    31/05/2017, 16:30
  8. 53. The Pierre Auger Observatory: recent results and prospects
    Lorenzo Cazon (LIP)
    31/05/2017, 16:50
  9. 49. Gravitational waves from the asymmetric dark matter generating phase transition
    Iason Baldes
    31/05/2017, 17:10
  10. 50. Results and prospects for BICEP3/Keck
    John Kovac
    31/05/2017, 17:30
  11. 51. Results and prospects from SPTpol and SPT-3G
    Amy Bender
    31/05/2017, 17:50
  12. 52. Cosmological results from the Kilo Degree Survey
    Hendrik Hildebrandt (Univ. Bonn)
    31/05/2017, 18:10
  13. 64. High-resolution SZ cartography of clusters of galaxies with the NIKA2 camera at the IRAM 30-m telescope
    Frédéric MAYET (CNRS)
    31/05/2017, 18:30
  14. 65. Neutrinos in Cosmology
    Eleonora Di Valentino
    31/05/2017, 18:50
  15. 56. Cosmic Microwave Background Measurements with the South Pole Telescope
    Amy Bender (Argonne National Laboratory)
    Oral

    The South Pole Telescope (SPT) is a millimeter-wavelength telescope surveying the cosmic microwave background (CMB). The SPT measures both the temperature and polarization of the CMB with a large aperture, resulting in high-resolution maps sensitive to signals across a wide range of angular scales on the sky. With these capabilities, the SPT has the potential to constrain inflationary...

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  16. 55. Cosmological results from H0liCOW
  17. 47. Cosmological results from the Kilo Degree Survey
    Hendrik Hildebrandt (Univ. Bonn)
    Oral

    Gravitational lensing represents a unique tool to study the dark Universe. In the weak lensing regime small distortions in the images of galaxies caused by the large-scale structure can be detected over the whole sky. Measuring these coherent distortions yields cosmological insights complementary to other probes like the cosmic microwave background (CMB). Ongoing wide-field imaging surveys...

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  18. 61. High-resolution SZ cartography of clusters of galaxies with the NIKA2 camera at the IRAM 30-m telescope
    Frédéric Mayet (Université Grenoble Alpes)
    Oral

    Arcmin resolution thermal Sunyaev-Zeldovich (tSZ) observations (e.g. SPT, ACT and Planck) only allowed detailed studies of the intra cluster
    medium morphology for low redshift clusters (z < 0.2).
    The development of precision cosmology with clusters requires high-angular resolution observations to extend the understanding of galaxy clusters towards high redshift. NIKA2 is a wide-field (6.5...

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  19. 67. tba
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