IR Retreat 2007 (Dec 10-12)
Kloster Seeon
The basic idea is to use this get together for focussing on/discussing possible future projects and science.  
Speakers should make their presentations as short as possible - the goal of the presentations is to stimulate discussion - the listed times include discussion!!!
Not everyone is giving a presentation, but everyone should come prepared for discussion in at least 1 of the topics.
Monday Dec 10th
Session Time Duration Speaker Title/Event
Transport, arrival, logistics 08:15 bus leaves front of MPE
10:00 ARRIVAL AT SEEON AND CHECK-IN
10:30 00:05 Linda Tacconi welcome
10:35 00:30 Reinhard Genzel Setting the Scene - Strategies for the Retreat
TOPIC I: IR Group Projects Coordinator: Reiner Hofmann
1) Overview of projects 11:05 00:15 Reiner Hofmann Overview
nearing completion 11:20 00:30 Peter Buschkamp LBT + LUCIFER, status, schedule, performance
11:50 00:20 Oliver Pfuhl PRIMA, concept, status, schedule, performance
12:10 00:30 Albrecht Poglitsch Herschal/PACS, status, schedule, performance
12:40 00:20 Mario Schweitzer SOFIA + FIFFI-LS, status, schedule, performance
13:00 01:15 LUNCH
2) Projects Under Development 14:15 00:30 Ric Davies KMOS, concept, status, MPE involvement
14:45 00:20 Sebastian Rabien LBT Laser Guide Star, concept, status, MPE involvement
15:05 00:30 Stefan Gillessen GRAVITY, concept, status, MPE involvement
15:35 00:20 Ric Davies E-ELT MCAO Camera, concept, MPE involvement
3) Prjoects in Planning Phase 15:55 00:20 Francisco Mueller-Sanchez SERPIL-LINUS, concept, status
16:15 00:30 COFFEE BREAK
16:45 00:40 Lothar Strueder BIB-type Si:Sb arrays and Wavefront Sensors, Activities of the HLL
17:25 00:30 Walfried Raab SPICA, concept, status, MPE involvement
17:55 00:30 Frank Eisenhauer DUNE, concept, status, MPE involvement
19:00 DINNER
20:00 01:30 Coordinators: Ric Davies, Sascha Trippe Managing a PhD
Tuesday Dec 11th
Session Time Duration Speaker Title/Event
08:00 BREAKFAST
Topic II: Science Planning for
Herschel PACS GTO Programs Coordinator: Dieter Lutz
Format considerations:        
Few introductory/framework talks. Major part will be devoted to topical presentations of science cases with the goals of:
1) sharpening our view of science priorities      
2) identifying loose ends in ancillary data/model availability and follow up needs  
3) Outlining path from survey data to science      
Each of these should address without too much ado:    
1) goal and why it is important        
2) status (e.g. spitzer)        
3) path to result: which field do you use, what ancillary data, models etc.  
1) Surveys: Introduction 09:00 00:30 David Elbaz Status and issues in extragalactic infrared surveys
09:30 00:20 Dieter Lutz GTO extragalactic surveys overview
09:50 00:20 Paola Andreani Herschel/Alma extragalactic synergies
2) Surveys: Science Cases 10:10 00:20 Stefano Berta Resolving the CIB
10:30 00:30 COFFEE BREAK
11:00 00:20 Paola Popesso Star formation as a function of environment
11:20 00:20 Dieter Lutz Coexistence of AGN and star formation
11:40 00:20 Natascha Foerster Schreiber Infrared emission of known high z populations
12:00 00:20 Emanuele Daddi Search for very high z starbursts
12:20 01:40 LUNCH
3) Surveys: Science Cases and 14:00 00:20 Paola Andreani PEP and obscured Spitzer sources
Wrapup Discussion 14:20 00:20 Nicolas Bouche Clustering of Herschel surces and correlation with other populations
14:40 00:20 Andrea Cimatti Early-type galaxies at high z
15:00 00:20 Linda Tacconi Millimeter studies of Herschel sources
15:20 00:30 All DISCUSSION: Science priorities for PEP
15:50 00:30 COFFEE BREAK
4) Spectroscopy of Nearby 16:20 00:30 Eckhard Sturm PACS spectroscopy of bright galactic nuclei: Overview
and Distant Galaxies 16:50 00:25 Alessandra Contursi Herschel and the CII deficit
17:15 00:25 Jackie Fischer Herschel and molecules in ULIRGs
17:40 00:25 Javier Gracia-Carpio High z spectroscopy with PACS
18:05 00:15 All DISCUSSION: Science priorities for spectroscopy
19:00 DINNER
Evening Possible Topical Discussion or Free
Wednesday, Dec 12
Session Time Duration Speaker Title/Event
08:00 BREAKFAST
TOPIC III:
Future directions of
our high-z science program:
Coordinator: Natascha Foerster Schreiber See detailed description on web for more details about the session
and beyond
The speakers should explicitly address the following aspects:    
I. The scientific context, both theoretical and observational    
II. The impact of the results        
III. The open questions and the next steps to make progress    
IV. The bridge between SINFONI and LUCIFER    
V. Link the results/questions to the role of mass, gas, SF, feedback, environment, redshift evolution.  
1) SINS, LUCIFER 09:00 00:10 Natascha Foerster Schreiber Introduction Overview SINS, LUCIFER high-z science cases
and Related Observational 09:10 00:20 Kristen Shapiro Gas kinematics and implications I (kinemetry, nature of galaxies)
Results 09:30 00:20 Giovanni Cresci Gas kinematics and implications II (modeling, TFR)
09:50 00:20 Nicolas Bouche Dynamics (velocity-size, angular momentum), DM connection
10:10 00:30 Reinhard Genzel Gas, stars & star formation; mass accretion and galaxy growth
10:40 00:30 COFFEE BREAK
11:10 00:20 Natascha Foerster Schreiber Mass, metallicity, environment
11:30 00:20 Erin Strobel Hicks Black hole evolution at high z
11:50 00:20 Emanuele Daddi AGN vs star formation in high-z galaxies
12:10 01:30 LUNCH BREAK
2) Theoretical perspectives 13:40 00:15 Thorsten Naab Galaxy formation in L-CDM; baryons-DM connection
13:55 00:15 Shy Genel Role of mergers
14:10 00:15 Andi Burkert Disk formation and evolution
14:25 00:15 Peter Johansson Mergers & BH feedback
3) Synergies with other surveys 14:40 00:20 Linda Tacconi Synergies with submm
15:00 00:20 Dieter Lutz Synergies with Herschel
15:20 00:20 COFFEE BREAK
4) Summary and Discussion 15:40 01:00 All Discussion:
Science priorities for SINS & LUCIFER
Scientific impact assessment of planned programs
What does theory need? What do observations provide?
Scope expansion and role of other NIR instruments
(NACO, HST/NICMOS, WFC3, KMOS, JWST, etc.)
16:40 END OF SESSION
17:15 BUS LEAVES SEEON TO RETURN TO MPE