Unlocking the potential of JWST, Euclid, and SKA - high-z galaxy evolution and cosmology

→ Europe/Rome
205 (IFPU)

205

IFPU

Fabio Fontanot (Istituto Nazionale di Astrofisica (INAF)), Marta Spinelli (Istituto Nazionale di Astrofisica (INAF)), Peter Lustig (IFPU)
Description

Zoom link for the Meeting:

Topic: ifpugaea2023

 

Join Zoom Meeting

https://ethz.zoom.us/j/66803867823

 

Meeting ID: 668 0386 7823.

 

For in-person participants please refer to the image below for info on ICTP and IFPU location (courtesy of Matteo Biagetti).

    • 10:30 AM → 11:00 AM
      Welcome/Coffee 30m
    • 11:00 AM → 11:30 AM
      An overview of GAEA 30m 205

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      Speaker: Gabriella De Lucia (Istituto Nazionale di Astrofisica (INAF))
    • 11:30 AM → 12:00 PM
      An overview of GAEA (Multi-phase gas content) 30m 205

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      Remote

      Speaker: Dr Lizhi Xie
    • 12:00 PM → 2:00 PM
      Lunch at ICTP 2h
    • 2:00 PM → 2:30 PM
      An overview of GAEA (AGNs and Variable IMF) 30m 205

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      Speaker: Fabio Fontanot (Istituto Nazionale di Astrofisica (INAF))
    • 2:30 PM → 5:30 PM
      Discussion 3h 205

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    • 9:30 AM → 10:00 AM
      A non-universal IMF with updated stellar population models from FUV through NIR 30m 205

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      Speaker: Francesco La Barbera (Istituto Nazionale di Astrofisica (INAF))
    • 10:00 AM → 10:30 AM
      Q&A 30m 205

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    • 10:30 AM → 11:00 AM
      Coffee Break 30m 205

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    • 11:00 AM → 11:30 AM
      Quenching and morphological evolution of galaxies at z~3 30m 205

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      Speaker: Lustig Peter
    • 11:30 AM → 12:00 PM
      Q&A 30m 205

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    • 12:00 PM → 2:00 PM
      Lunch at ICTP 2h 205

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    • 2:00 PM → 2:30 PM
      Filaments in GAEA. Galaxies in Virgo cluster in observations and in GAEA 30m 205

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      Speaker: Daria Zacharova
    • 2:30 PM → 5:30 PM
      Discussion 3h 205

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    • 9:30 AM → 10:00 AM
      Galaxy populations in the first massive clusters 30m 205

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      Speaker: Veronica Strazzullo (Istituto Nazionale di Astrofisica (INAF))
    • 10:00 AM → 10:30 AM
      Q&A 30m 205

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    • 10:30 AM → 11:00 AM
      Coffee Break 30m 205

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    • 11:00 AM → 11:30 AM
      A (biased) view of JWST on galaxy evolution: First results from the GLASS survey 30m 205

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      Speaker: Benedetta Vulcani (Istituto Nazionale di Astrofisica (INAF))
    • 11:30 AM → 12:00 PM
      Q&A 30m 205

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    • 12:00 PM → 1:30 PM
      Lunch at ICTP 1h 30m 205

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    • 1:30 PM → 2:00 PM
      Identification and characterization of galaxy protoclusters in spectroscopic and photometric surveys 30m 205

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      Speaker: Olga Cucciati (Istituto Nazionale di Astrofisica (INAF))
    • 2:00 PM → 2:30 PM
      Q&A 30m 205

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    • 2:30 PM → 3:00 PM
      Optical emission-line predictions of galaxy populations in GAEA for the EUCLID Deep and Wide surveys 30m 205

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      Speaker: Lucie Scharré
    • 3:00 PM → 6:00 PM
      Dicussion 3h 205

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    • 9:30 AM → 10:00 AM
      The origin of supermassive black holes: implications for host galaxies from semi-analytical modelling 30m 205

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      Speaker: Vieri Cammelli
    • 10:00 AM → 10:30 AM
      Q&A 30m 205

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    • 10:30 AM → 11:00 AM
      Coffee Break 30m 205

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    • 11:00 AM → 11:30 AM
      Massive black hole binaries in the era of gravitational wave detectors: Could we constrain cosmology with them? 30m 205

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      Speaker: David Izquierdo
    • 11:30 AM → 12:00 PM
      Q&A 30m 205

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    • 12:00 PM → 2:00 PM
      Lunch at ICTP 2h 205

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    • 2:00 PM → 2:30 PM
      The Spiderweb protocluster rebooted 30m 205

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      Speaker: Maurilio Pannella
    • 2:30 PM → 3:00 PM
      Q&A 30m 205

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    • 3:00 PM → 3:30 PM
      GAEA for SKA Cosmology 30m 205

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      Remote

      Speaker: Marta Spinelli (Istituto Nazionale di Astrofisica (INAF))
    • 3:30 PM → 4:00 PM
      Q&A 30m 205

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    • 4:00 PM → 7:00 PM
      Discussion 3h 205

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    • 9:30 AM → 11:30 AM
      General Discussion (including coffee break and/or splinter sessions) 2h 205

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    • 11:30 AM → 12:00 PM
      Final Wrap-Up 30m 205

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    • 12:00 PM → 2:00 PM
      Lunch at ICTP 2h 205

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    • 2:00 PM → 5:00 PM
      End of Activities - Rooms and Desk available for follow-up discussions among participants 3h 205

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