Galaxies & AGN with the First Euclid data and beyond

Europe/Rome
Città della Scienza, Naples

Città della Scienza, Naples

Via Coroglio, 57/104, 80124 Napoli NA
Viola Allevato (Istituto Nazionale di Astrofisica (INAF))
Description

The Workshop is open ONLY to Euclid Consortium members

Euclid is going to be launch-ready by spring 2023, and hopefully actually launched not much further down the line. A call for Key Projects using actual Euclid data is forthcoming. This is excellent timing to start focusing on the scientific projects we would like to carry out with the Euclid data, as a collaboration, particularly in this case as part of the Galaxy and AGN Evolution Science Working group. 

We will meet for 3 days that will be dedicated to the presentation of science projects, with a large space left for discussions and sub-group/topical parallel sessions. This will be along the topics defined by the SWG Work-packages, dealing with star forming and passive galaxies, galaxy morphology, lensing, environment, AGN, distant galaxies, etc etc. But also beyond, and discussion of further applications and science ideas is welcome. 

SOC:

Viola Allevato (Chair), Jarle Brinchmann, Emanuele Daddi, Andrea Cimatti (co-chairs), Giovanni Covone, Lucia Pozzetti, Margherita Talia, Manuela Magliocchetti, Jenny Sorce, Marc Huertas-Company, Michele Moresco, Gabriella De Lucia, Alessandro Sonnenfeld, Sotiria Fotopoulou, Elena Zucca.

LOC

Maurizio Paolillo (Chair), Viola Allevato (co-chair), Crescenzo Tortora, Giovanni Covone, Demetra De Cicco, Olena Torbaniuk, Michele Delli Veneri, Rosario Aiello

The workshop will be held at Monte Sant'Angelo, Sala Azzurra in Naples, Italy on 14-16 September 2022.

NEW Agenda

 

Accommodation

We have a variety of accommodation possibilities in Naples, but please book early as middle of September is still "high season" in Naples. Every morning we will provide a shuttle leaving from Piazza Vittoria to the conference center and back from the conference center to Piazza Vittoria in the evening. We then suggest you to book your room within walking distance from Piazza Vittoria, a  beautiful front-sea area full of hotels, b&b/airb&b and restaurants.. 

You can also reach the conference center "Città della Scienza" by public transportation. Take the direct bus R7 from "Piazza Vittoria Riviera di Chiaia" towards "Bagnoli - La Pietra" and get off after 22 stops at "Coroglio - Città della Scienza". The ticket is 1.10 euros. You can download the App Unico Campania, available on Play Store and App Store , in Android and iOS version and use it to check the bus schedule, calculate the route and buy the ticket  after registering as new user.

Travelling to Naples

Reaching Naples is simple! 

By plane: the Naples' international airport (Napoli- Capodichino, NAP), is located less than 6 km northeast of the city center, with direct international flights arriving and departing daily. There is a regular bus service (Alibus Shuttle) from the airport to the centre of the town. A one-way ticket costs 5euros and takes you directly to Piazza Garibaldi in just 15 minutes. Taking a taxy may be more expensive, but it's definitely the most convenient. The journey shouldn't take more than 12 minutes and will cost you a flat rate fee of ~20 euros.

By train: Naples' main train stations is called Napoli Centrale (or Piazza Garibaldi Station) and both Trenitalia (Italian national rail company) and private Italo trains arrive and depart from here. 

Participants
  • Akke Viitanen
  • Alba Vega Alonso Tetilla
  • Alberto Cappi
  • Alberto Manjón-García
  • Aleksandar Shulevski
  • Anastasio Díaz-Sánchez
  • Andrea Francesco Maria Enia
  • Angelos Nersesian
  • Anthony Gonzalez
  • Antonio La Marca
  • Berta Margalef Bentabol
  • Bruno Altieri
  • Carlotta Gruppioni
  • Chiara Mancini
  • Clotilde Laigle
  • Crescenzo Tortora
  • Daniela Vergani
  • Darko Donevski
  • Demetra De Cicco
  • Diana Scognamiglio
  • Douglas Scott
  • Elisabeta Lusso
  • Emanuele Daddi
  • ENRICHETTA IODICE
  • Fabio La Franca
  • Filippo Mannucci
  • Florian Sarron
  • Francesco Shankar
  • Francisco Javier Castander
  • Gabriella De Lucia
  • Gary Mamon
  • Giovanni Covone
  • Giulia Rodighiero
  • Grant Stevens
  • Hao Fu
  • Igor Zinchenko
  • ISABELLA PRANDONI
  • Jarle Brinchmann
  • Jean-Charles Cuillandre
  • Jenny Sorce
  • John Silverman
  • Jon Loveday
  • Knud Jahnke
  • Laura Bisigello
  • Lingyu Wang
  • louis gabarra
  • Lucia Pozzetti
  • Maarten Baes
  • Manuela Magliocchetti
  • Marco Mignoli
  • Marco Scodeggio
  • Marco Tucci
  • Margherita Talia
  • Marilena Spavone
  • Marko Shuntov
  • Martin Sahlén
  • Marziye Jafariyazani
  • Matthew Selwood
  • Matthieu Bethermin
  • Maurizio Paolillo
  • Meriam Ezziati
  • Michael Balogh
  • Michele Cirasuolo
  • Michele Delli Veneri
  • Michele Moresco
  • Micol Bolzonella
  • Mohammad Kamran
  • Nicola Malavasi
  • Nicole Nesvadba
  • Olena Torbaniuk
  • Olga Cucciati
  • Oscar Chavez Ortiz
  • Paola Dimauro
  • Pascale Jablonka
  • Pedro Cunha
  • Rebecca Bowler
  • Rees Williams
  • Roberto Maiolino
  • Rosemary Coogan
  • Roser Pello
  • Salvatore Quai
  • Sandor Kruk
  • Sandy Morais
  • Seunghwan Lim
  • Simona Mei
  • Sophie Maurogordato
  • Sotiria Fotopoulou
  • Stefan Hackstein
  • Stéphane Paltani
  • Theosamuele Signor
  • Tohru Nagao
  • Ulrike Kuchner
  • Veronica Strazzullo
  • Vincenzo Petrecca
  • Viola Allevato
  • Xavier Lopez Lopez
  • Yoshiki Toba
Viola Allevato
    • Day 1: Plenary Session 1
      • 1
        Welcome + SWG-GEV Leads
      • 2
        OU-PHZ (S. Paltani)
      • 3
        Science Archive (B. Altieri)
      • 4
        LSST - UNIONS (J. C. Cuillandre)
      • 5
        Discussion plenary 1
      • 11:00
        Coffee Break
    • Day 1: Plenary Session 2
      • 6
        S.Lim - CIB-COB imaging cross-correlation and constraints on galaxy formation
      • 7
        M. Shuntov - Magnification as a probe of halo masses
      • 8
        Discussion: Multi-wavelength synergies (M. Bethermin)
      • 9
        Discussion: Follow-up observations
      • 12:45
        Lunch Break
    • Day 1: Plenary Session 3: Environment
      • 10
        N. Malavasi - Characterizing the detection of the cosmic web
      • 11
        R.Coogan - Multi-wavelength detection of high-z overdensities
      • 12
        C. Laigle - Measuring the 2D alignments between galaxies and their cosmic web environment in EDFs
      • 13
        P. Dimauro - Intracluster light detection at high-z
      • 14
        G.Mamon - How well can Euclid measure evolution of color segregation with density profiles
      • 15
        S. Mei - Galaxy Scaling Relations in clusters at z>1.5
      • 16
        A. Diaz-Sanchez - Detection of cluster & protocluster using CARTHAGO algorithm
      • 16:00
        Coffee Break
    • Day 1: Parallel Session b: WP4
    • Parallel Session c: Spectroscopy
      • 17
        Spectral Stacking (E. Lusso)
      • 18
        Discussion on spectral stacking
      • 19
        Updates on simulations (M. Scodeggio, C. Mancini)
      • 20
        Discussion
    • Day 1: Parallel session a: WP3
    • DAY 2: Plenary Session 4
      • 21
        OU-SPE (M. Moresco)
      • 22
        SWG - LU (C. Tortora)
      • 23
        SWG - PU (J. G. Cuby)
      • 24
        Flagship (F. Castander)
      • 25
        Discussion plenary 4
      • 11:00
        Coffee Break
    • Day 2: Plenary Session 5
      • 26
        G. De Lucia - Galaxy Mocks for legacy science
      • 27
        C. Mancini - Euclid forecasts for galaxy evolution
      • 28
        L. Pozzetti - Census of overweight galaxies with Q1-DR1
      • 29
        M. Bolzonella - Bulk galaxy properties and unconventional objects from Q1 and DR1
      • 30
        Discussion plenary 5
      • 13:00
        Lunch Break
    • Day 2: Plenary Session 6
      • 31
        M.Baes - Extracting the distribution of stellar mass, age and metallicity in nearby galaxies
      • 32
        D. Donevski - Unveiling the nature of dusty quiescent galaxies
      • 33
        O. Chavez Ortiz - Using Euclid to explore correlations between galaxies and emergent Lyman-alpha strength
      • 34
        S. Kruk - The evolution of the internal structures of galaxies with Euclid
      • 35
        D. Scognamiglio - Searching for ultra compact massive galaxies
      • 36
        R. Bowler - Prospects for studying luminous galaxies in the EoR
      • 37
        S. Theosamuele - High z galaxies identification in the EDFs
      • 16:15
        Coffee Break
      • 38
        M. Ezziati - The selection of high-z quasars
      • 39
        M. Selwood - Expected number of AGN
      • 40
        F. Mannucci - Detection dual/lensed AGN at small separations
      • 41
        Discussion plenary 6
    • Day 3: Plenary Session 7
      • 42
        4MOST (J. Loveday)
      • 43
        WEAVE (U. Kuchner)
      • 44
        MOONS (M. Cirasuolo)
      • 45
        IR Surveys (C. Gruppioni)
      • 46
        Discussion Plenary 7
      • 11:00
        Coffee Break
    • Day 3: Plenary Session 8
      • 47
        J.Silverman - Connections between SMBHs, host galaxies and their DMHs
      • 48
        H.Fu - Impact of the stellar mass-halo mass relation in galaxy merger
      • 49
        F. Shankar - Constraints on the assembly histories of galaxies and SMBHs
      • 50
        X. Lopez - Exploitation of AGN in Euclid Q1/DR1 with an empirically generated catalog
      • 51
        Discussion Plenary 8
      • 13:05
        Lunch Break
    • Day 3: Plenary Session 10: Photometry
      • 52
        A. Enia - Characterizing the evolution of galaxy physical properties relation with machine learning
      • 53
        L. Bisigello - Selecting AGN using observed Euclid colors
      • 54
        Discussion: Galaxies
      • 55
        Discussion: AGN
    • 16:00
      Coffee Break
    • Day 3: Plenary Session 9: Spectroscopy
      • 56
        L. Gabarra - Euclid PILOT spectral simulations
      • 57
        M. Jafariyazani - Self Organizing Maps as a tool to infer spectroscopic features of galaxies from their broadband colors
      • 58
        Discussion: galaxies
      • 59
        Discussion: AGN