Grenoble,
France
NEW: presentations are
now available in the program section
09:00 | Welcome |
09:30 | Introduction
to the NEAT proposal - F.
Malbet (IPAG, Obs. Grenoble,
France): Concept,
performance, scaling, parameter space,
programmatics
|
10:00 | Science case 1 (1.5h): Constraints
for the formation of planetary systems and
orbits evolution Chairman : R. Liseau (Chamlers Univ. of Technology, Gothenburg, Sweden) Panel discussion: - Y.
Alibert (Univ. Bern, Switzerland):
Constraints
for the formation of planetary sysytems
- A. Crida (OCA, Univ. Nice, France): Formation of the Solar System - J. Laskar (IMCCE, Obs. Paris, France): Dynamics of planetary systems in interaction - H. Beust (IPAG, Obs. Grenoble, France): Orbit evolution of planetary systems |
11:30 | Science
case 2 (1.5h): Identification of
Terrestrial planets in the habitable zone of
nearby solar-type stars Chairman : C. Eiroa (Univ. Madrid, Spain) Panel discussion: - C.
Eiroa (Univ. Madrid, Spain): Introduction
- A. Léger (IAS, Univ. Paris-Sud, Orsay, France): Identification of Terrestrial Planets> - M. Shao (Jet Propulsion Laboratory, Pasadena, USA): ExoEarth Target Lists: How Many Stars Need to be Searched? How Large a Telescope is Needed? - D. Queloz (Obs. Geneva, Swizterland): Pushing down the limits - W. Traub (Jet Propulsion Laboratory, Pasadena, USA): Terrestrial Habitable‐Zone Exoplanet Frequency from Kepler |
13:00 | Lunch buffet (1h) |
14:00 | Science
issues (1h) Chairman : A. Léger (IAS, Univ. Paris-Sud, Orsay, France) Panel discussion: - N.
Meunier (IPAG, Obs. Grenoble,
France): Impact
of stellar activity on radial velocities and
astrometry
- M. Shao (Jet Propulsion Laboratory, Pasadena, USA): Multiple planets in reference stars - F. Malbet (IPAG, Obs. Grenoble, France): Activity of background reference K giants |
15:30 | Science case 3 (1.5h): diversity
of exoplanets (different stellar hosts, various
ages, types of planets,...) Chairman D. Queloz (Obs. Geneva, Swizterland) Panel discussion: - A.-M.
Lagrange (IPAG, Obs. Grenoble,
France): A
stars and planet formation
- D. Ségransan (Obs. Geneva, Swizterland) / X. Bonfils (IPAG, Obs. Grenoble, France): About M stars - D. Defrère (MPIfR, Bonn, Germany): Debris disks - E. Villaver (Univ. Madrid, Spain): Evolved stars: Planets orbiting the other stellar systems: Giant Stars White Dwarfs? - F. Malbet (IPAG, Obs. Grenoble, France): The case of Young Stars |
16:30 | Science
case 4 (1.5h): additional science
cases Chairman A. Quirrenbach (Univ. Heidelberg, Germany) Panel discussion : - A.
Quirrenbach (Univ. Heidelberg,
Germany): Additional
science: boon or bane?
- T. Maschberger (IPAG, Obs. Grenoble, France): Young stellar cluster dynamics - D. Hestroffer (IMCCE, Obs. Paris, France): Astrometry of Solar System Objects - G. Dubus (IPAG, Obs. Grenoble, France): Compact galactic objects - M. Shao (Jet Propulsion Laboratory, Pasadena, USA): Another Application of micro-arcsec Astrometry of Asteroids |
18:00 | Other
contributions Oral presentations: - E.
Plávalová (Comenius University,
Bratislava, Slovakia): Taxonomy
of the extra-solar planets
- D. Chen (National Space Science Center, CAS, Beijing, China): Space Astrometry Telescope - pathfinder for the future universe mearsurement |
20:00 | Workshop dinner |
09:00 | NEAT instrument proposal
(2h): Chairman: L. Labadie (I. Physikalisches Institut, Cologne, Germany) Panel discussion: - M.
Shao (Jet Propulsion Laboratory,
Pasadena, USA): Main requirements
for ultra-high precision differential
astrometry
- F. Malbet (IPAG, Obs. Grenoble, France): Payload concept - A. Crouzier (IPAG, Obs. Grenoble, France): Designing a testbed for micropixel centroid measurement - R. Goullioud (Jet Propulsion Laboratory, Pasadena, USA): Design and Specificaons - Questions/Discussion |
11:00 | Instrument/Mission discussion
(2h): Chairman: P.-O. Lagage (CEA/Sap AIM, Saclay, France) Panel discussion: - L.
Labadie (I. Physikalisches
Institut, Cologne, Germany): Scaling
options for NEAT
- E. Hinglais (CNES, Toulouse, France): Trade off: Formation Flying vs. Mast for space distributed instrumentation purpose - B. Jakobsson (OHB Sweden, Solna, Sweden): Instrument & Mission / Available Tech, PRISMA relateds (video #1, video #2, video #3) - R. Goullioud (Jet Propulsion Laboratory, Pasadena, USA): Error budget and scaling - Ph. Feautrier (IPAG, Obs. Grenoble, France): NEAT Detector requirements - D. Hobbs (Lund Observatory, Lund, Sweden): Effects of radiation damage - M. Shao (Jet Propulsion Laboratory, Pasadena, USA): Scattered Light Issues Deployed and Free Flyers - A. Léger (IAS, Univ. Paris-Sud, Orsay, France): Mission operation: number of visits - Questions/discussion |
13:00 | Lunch buffet (1h) |
14:00 | Discussion of possible actions
(2h): Double Blind test study (1h) Chairman: W. Traub (Jet Propulsion Laboratory, Pasadena, USA) Introduction talk: NEAT Double-Blind Considerations: Experience from SIM Panel: A. Léger (IAS, Univ. Paris-Sud, Orsay, France), A.-M. Lagrange (IPAG, Obs. Grenoble, France), G. Duvert (IPAG, Obs. Grenoble, France) NEAT precursors: balloon experiment, smaller mission,... for which science (1h) Chairman: D. Mouillet (IPAG, Obs. Grenoble, France) Panel: B. Jakobsson (OHB Sweden, Solna, Sweden), M. Shao (Jet Propulsion Laboratory, Pasadena, USA) |
16:00 | List of actions and conclusion
of the workshop (1h) F. Malbet (IPAG, Obs. Grenoble, France): First conclusions |
17:00 | End of the workshop |
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The
PDF document gives the indications how to reach
IPAG (Grenoble) and provides a list of recommended
hotels.