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In this virtual meeting we will focus especially on the Yellow Book preparation. In particular we need to revise the allocated sections in the v0.39 PDF distributed last July. The structure will be made of a shorter introduction (max 3 pages), fewer figures, followed by the list of the sections:
2.1.1 Tracking the drivers for galaxy evolution over cosmic time —introduction and figures
2.1.2 Gaining the full 3D perspective on Star Formation and Black Hole accretion
2.1.3 Establishing the role of obscured BH-growth in the evolution of galaxies
2.1.4 Characterising the feedback mechanisms that quench Star Formation
2.1.5 Tracing the build-up of Heavy Elements over the last 10 Gyr
2.1.6 Following dust evolution from reionization to the present-day Universe
- The first day will be dedicated to the presentation of the various sections of the WB: 10 min. presentation, followed by 20 min. discussion. Later in the afternoon we will have a discussion on the best figures to be implemented.
- The second day will be dedicated to splinters on each topic, where the various groups will actually work together on the text.
- The third day the reports from each splinter will be given and discussed.
- The last afternoon we have a special session dedicated to the updates on the white papers in preparation.
The meeting will occupy the mornings (9:00-11:30am CEST) and the afternoons (4:00-6:30pm CEST) from Monday 5th to Wednesday 7th.
Participants List
Preliminary Programme of the SPICA GalEvol Virtual meeting
[Download Programme PDF]
Programme of the SPICA GalEvol Virtual meeting
First Day: Monday 5th October 2020
8:45 meet with a zoom connection Join Zoom Meeting
9:00 – 9:10: Introduction to the Galaxy Evolution SPICA science cases
The draft GalEvol YB chapter: structure and key aspects
9:10 – 9:20
presentation and discussion on the introduction:
Luigi – 2.1.1 Tracking the drivers for galaxy evolution over cosmic time
9:20 – 9:40 – discussion
9:40 – 9:50 Alberto/Giulia -2.1.2 Gaining the full 3D perspective on star formation and black hole accretion
9:50 – 10:10 – discussion
10:10 – 10:20 virtual coffee
10:20 – 10:30 Francesca/Cristian 2.1.3 Establishing the role of obscured BH-growth in the evolution of galaxies
10:30 – 10:50 – discussion
10:50 – 11:00 Simona/Eiichi 2.1.6 Following dust evolution from re-ionization to the present day Universe
11:30 end of first session
4:00 – 4:10 Jackie 2.1.4 Characterising the feedback mechanisms that quench Star Formation
4:10 – 4:30 – discussion
4:30 – 4:40 Juan 2.1.5 Tracing the build-up of Heavy Elements over the last 12 Gyr
4:40 – 5:00 – discussion
5:00 – 5:10 break
5:10 – 6:10 Discussion on the figures
6:10 – 6:30 Wrap up
6:30 end of second session
Second Day: Tuesday 6th October 2020
9:00 – 11:30 Splinters on various WP:
topic 1: 3D perspective
topic 2: feedback
topic 3: obscured BH-growth
topic 4: metallicity evolution
topic 5: dust evolution from re-ionization – high-z studies
11:30 end of third session
4:00 – 5:00 Continued splinters on various WP:
topic 1: 3D perspective
topic 2: feedback
topic 3: obscured BH-growth
topic 4: metallicity evolution
topic 5: dust evolution from re-ionization – high-z studies
6:30 end of fourth session
Third Day: Wednesday 7th October 2020
9:00 – 10:15 Reports from topics 1, 2,3
10:15 – 10:25 break
10:25 – 11: 30 Reports from topics 4, 5
11:30 end of fifth session
4:00 – 5:00 Final Discussion: list of actions of written contributions of the YB
5:00 – 5:10 break
5:10 – 6:30 White papers presentations: updates following the new telescope configuration and the lack of CAM34
- Luigi Branchiesi (PhD student in Bologna Univ.): SPICA/Athena synergies
- Laura Bisigello (Postdoc at OAS-INAF, Bologna): mock catalog to predict SPICA detections
- Giulia Rodighiero (TBD): clustering studies
- Laure Ciesla: How to make the most of SPICA data, with statistics and machine learning techniques
- Juan Antonio Fernández-Ontiveros: new method to measure metallicities through the IR lines
- Simona Gallerani: by reviewing the work done in her team at SNS for SPICA predictions and simulations
6:30 end of sixth and final session
contact people:
j.a.fernandez.ontiveros [at] gmail.com
luigispinoglio [at] gmail.com
Monday 18th May 2020
8:30 meet with a zoom connection TBD
8:45 – 9:00: Welcome and introduction to the Yellow Book – Peter Roelfsema
9:00 – 9:30: Introduction to the Galaxy Evolution SPICA science cases – David
9:30 – 9:40: The draft GalEvol YB chapter: how it has been structured, what are the “bullets” – [Lee (tbc)/David/Juan/Luigi]
[Note: each topic will have: 10 min. intro. + key questions and key figures - identify actions on what needs to be implemented]
The hidden physics driving the evolution of galaxies:
day 1 – 3D view of galaxy evolution & Dark Matter halo – Magnetic Fields
9:40 – 10:30: What is the role of environment and clustering in shaping galaxy evolution? What is the role of obscured star-formation in building the most massive galaxy clusters that we observe today? [Giulia]
A white paper project will be on the presented by Giulia Rodighiero (TBD) for the clustering studies*
10:30 – 11:00: 3-D view of galaxy evolution: goals and implementation [Giulia]
Discussion about implementation plan: Shallow Survey
11:00 – 11:10 virtual coffee
11:10 – 12:00: How do the magnetic fields in galaxies evolve across cosmic times? How polarized is the dust emission of high-z dusty systems? Is there alignment between the polarization (and magnetic field) inside the cosmic web and/or between close neighbors? [Matthieu]
12:00 – 13:00: Simulations for SPICA predictions of photometric and spectroscopic surveys [Carlotta]
Laura Bisigello (Postdoc at OAS-INAF, Bologna) will present a white paper project on the use of a moc catalog to predict SPICA detections*
Laure Ciesla will present the idea of a white paper to investigate the techniques to make the maximum of SPICA data, photometric data for a start*
16:00 – 17:00: Brief summary of morning session and discussion with the American team [Lee, Asantha, Matt M.]
Tuesday 19th May 2020
The hidden physics driving the evolution of galaxies:
day 2 – Star Formation vs AGN coevolution, quenching, feedback, obscured AGN
10:00 – 11:00: What physical processes led to the peak star formation and black hole growth in the Universe at z ~ 2, known as the cosmic noon, and the rapid quenching of star formation in galaxies at z < 1? [Alberto F.]
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11:00 – 11:30: Obscured BH-growing phases in shaping galaxy evolution? [Francesca]
11:30 – 11:40 virtual coffee
11:40 – 12:30: How are star formation and black hole growth linked over cosmic time, what determines the tight relation between the mass of the SMBH and host galaxies seen in the local Universe, and are energetic outflows from supernovae and AGN responsible for the large mismatch in the stellar and dark matter halo mass functions? [Eduardo]
12:30-12:45 Luigi Branchiesi (PhD student in Bologna Univ.) will present a white paper project on the SPICA/Athena synergies*
12:45-13:00 Sabrina Mordini (PhD student at IAPS, Roma) presentation of the white paper draft: SPICA mid-IR cosmological spectrophotometric surveys: Measuring AGN and star formation at the Cosmic Noon*
16:00 – 17:00: Nearby galaxies discussion: how to include the topics within the galaxy evolution scheme? [Jesus, Floris, Sue, Vianney, Alberto B., Hidehiro]
life cycle of galaxies: how we integrate in the GalEvol scheme?
Wednesday 20th May 2020
The hidden physics driving the evolution of galaxies:
day 3 – baryon cycle & chemical evolution
09:00 – 10:00: What is the history of heavy elements and dust production in galaxies across cosmic time? How does accretion and the recycling of metals and dust drive the baryon cycle between galaxies and the CGM? [Juan]
A white paper project is going to be presented by Juan Antonio Fernandez-Ontiveros on a new method to measure metallicities through the IR lines that SPICA will observe*
10:00 – 11:00: What are the physical properties of star-forming galaxies and quasars in the epoch of reionization? [Simona]
A white paper project is going to be presented by Simona Gallerani by reviewing the work done in her team at SNS for SPICA predictions and simulations*
11:00 – 11:10 virtual coffee
11:10 – 13:00: Yellow Book final implementation discussion [David, Kotaro, Tohru, Luigi]
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16:00 – 17:00: Summary and discussion with the American team [Lee, Asantha, Matt M.]
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*We invite the white papers presenters to organize telecons open to the GalEvol WG members to discuss the implementation of the white papers.