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

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)

59. ANTARES highlights and KM3NET/ARCA prospects

Sergio Navas Concha (Universidad de Granada (ES))

31/05/2017, 14:00

60. Astrophysical neutrinos at IceCube, a new window to the Cosmos

Mohamed Rameez (NBI Kopenhagen)

31/05/2017, 14:20

45. Results from ARIANNA

Allan Hallgren (Uppsala University)

31/05/2017, 14:40

95. The Very-High-Energy Gamma-ray Sky: Recent Results from VERITAS

Elisa Pueschel (DESY)

31/05/2017, 15:00

48. Results from H.E.S.S.

Francois Brun (CENBG, Bordeaux)

31/05/2017, 15:20

66. Exploring the cosmic middle age with MAGIC

Dr Giacomo Bonnoli (Università degli Studi di Siena & INFN Pisa)

31/05/2017, 15:40

44. The Einstein@Home Gamma-ray Pulsar Survey

Colin Clark (AEI Potsdam)

31/05/2017, 16:30

53. The Pierre Auger Observatory: recent results and prospects

Lorenzo Cazon (LIP)

31/05/2017, 16:50

49. Gravitational waves from the asymmetric dark matter generating phase transition

Iason Baldes

31/05/2017, 17:10

50. Results and prospects for BICEP3/Keck

John Kovac

31/05/2017, 17:30

51. Results and prospects from SPTpol and SPT-3G

Amy Bender

31/05/2017, 17:50

52. Cosmological results from the Kilo Degree Survey

Hendrik Hildebrandt (Univ. Bonn)

31/05/2017, 18:10

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

65. Neutrinos in Cosmology

Eleonora Di Valentino

31/05/2017, 18:50

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...

55. Cosmological results from H0liCOW

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...

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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