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3° Meeting Nazionale Collaborazione Euclid

10–12 Feb 2020
CNR - Area della Ricerca di Bologna
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Session

Legacy Science

12 Feb 2020, 09:00
CNR - Area della Ricerca di Bologna

CNR - Area della Ricerca di Bologna

Via Piero Gobetti 101 - 40129 Bologna, Italia

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  1. 48. High-redshift cosmology with oxygen lines from Hα surveys
    Jose' C. Fonseca
    12/02/2020, 09:00
  2. 49. Simulating cosmological models beyond LCDM: current status and future prospects
    Marco Baldi
    12/02/2020, 09:12
  3. 50. Painting galaxies in mock samples for Euclid and future surveys
    Giacomo Girelli
    12/02/2020, 09:24
  4. 51. Science from CMB-galaxy cross-correlation
    Massimiliano Lattanzi
    12/02/2020, 09:36
  5. 52. Weak-lensing cross-covariances with non-primary probes in massive neutrinos cosmologies
    Matteo Calabrese
    12/02/2020, 09:48
  6. 53. Measuring lensing ratios with future cosmological surveys
    Bermejo Clement Jose
    12/02/2020, 10:00
  7. 54. Void statistics in dynamical DE models
    Giovanni Verza
    12/02/2020, 10:35
  8. 55. Cosmic void abundance as powerful additional probe for Euclid
    Sofia Contarini
    12/02/2020, 10:45
  9. 56. Correlations of cosmic voids with CMB maps in Large Scale simulations
    Pauline Vielzeuf
    12/02/2020, 10:55
  10. 57. Void-Lensing Cross-Correlation
    Marco Bonici
    12/02/2020, 11:05
  11. 58. Combined questions on void talks
    12/02/2020, 11:15
  12. 27. EC Scientific and editorial organization: overview and status of pre-launch KP definition
    Luigi Guzzo
    12/02/2020, 11:20
  13. 28. Questions/Discussion related to science projects, KPs, papers, etc.
    12/02/2020, 11:40
  14. 40. LSST & Euclid: the italian role
    Adriano Fontana
    12/02/2020, 12:10
  15. 29. Perspective summary talk: Euclid and the Future of Cosmology
    Stefano Borgani
    12/02/2020, 12:30
  16. 26. Contributed Scientific Talk: Highlights from all Cosmology SWGs (including non-primary probes)

    six 15-minute talks to be proposed by consortium members

    Go to contribution page
  17. 25. Introduction of Legacy Science Session
  18. 41. SWG Clusters
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