Scientific Programme
Day 2, Friday, Oct. 9 | ||
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08:30-09:00 |
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Registraton |
09:00-09:15 |
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Welcome Addresses |
09:15-10:15 | Roberto Gilmozzi |
The E-ELT precursor(s) |
10:15-11:00 | Suzanne Ramsay |
Science drivers for the E-ELT |
11:15-11:45 | Coffee Break | |
11:45-12:45 | Livia Origlia |
HIRES and extrasolar planets |
12:45-13:45 | Roberto Ragazzoni |
Adaptive optics: past present and future |
13:45-15:30 | Lunch | |
15:30-16:30 | Santi Cassisi |
Synthetic color magnitude diagrams: ingredients
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16:30-17:30 | Tom Herbst |
Detectors past, present and future |
17:30-18:00 | Tea Break | |
18:00-19:00 | Patricia Sanchez-Blasquez |
Unresolved Stellar Populations in the E-ELT era
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Day 3, Saturday, Oct. 10 | ||
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09:00-10:00 | Roberto Gilmozzi |
E-ELT and the future |
10:00-11:00 | France Allard |
Indirect Imaging of Ultra-Cool Dwarfs |
11:00-11:30 | Coffee Break | |
11:30-12:30 | Tom Herbst |
Detectors past present and future |
12:30-13:30 | Laura Schreiber |
Mapping the PSF across Adaptive Optics images |
13:30-15:30 | Lunch | |
15:30-16:30 | Simone Esposito |
SCAO pros and cons |
16:30-17:30 | Fiorentino/Schreiber
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Tutorial: Guess Who?
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17:30-18:00 | Tea Break | |
18:00-19:00 | Sebastian Kamann |
Introduction to Integral Field Spectroscopy
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Day 4, Sunday, Oct. 11 | ||
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09:00-10:00 | Enrico Marchetti |
MCAO past present and future |
10:00-11:00 | Roberto Ragazzoni
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11:00-11:30 | Coffee Break | |
11:30-12:30 | Patricia Sanchez-Blazquez |
Unresolved Stellar Populations in the E-ELT era |
12:30-13:30 | Bruno Leibundgut |
Supernovae Cosmology |
13:30-15:30 | Lunch | |
15:30-16:30 | Andrew Shearer |
High time resolution science and technology in the E-ELT era
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16:30-17:30 | Suzanne Ramsay |
E-ELT Instrumentations
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17:30-18:00 | Tea Break | |
18:00-19:00 |
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Students' talks |
Day 5, Monday, Oct. 12 | ||
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09:00-10:00 | Benoit Carry |
Solar system in the E-ELT era |
10:00-11:00 | Maurizio Salaris |
Advanced evolutionary phases current status and open problems |
11:00-11:30 | Coffee Break | |
11:30-12:30 | Enrico Marchetti
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MCAO past present and future |
12:30-13:30 | Jochen Liske |
Precision cosmology in the E-ELT era |
13:30-15:00 | Lunch | |
15:00-15:30 |
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Students' talks
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15:30-16:30 | Norbert Przybilla |
Blue super-giants in the E-ELT era
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16:30-17:30 | Fabrizio Fiore |
AGN & SN feedback: from galaxy evolution to the reionization epoch |
17:30-18:00 | Tea Break | |
18:00-19:00 | Origlia |
Spectroscopy of stars and stellar populations: from spectra to chemical abundances |
20:00 |
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Social Dinner |
Day 6, Tuesday, Oct. 13 | ||
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09:00-10:00 | Jochen Liske |
Precision cosmology in the E-ELT era |
10:00-11:00 | France Allard |
Indirect Imaging of Ultra-Cool Dwarfs |
11:00-11:30 | Coffee Break | |
11:30-12:30 | Benoit Carry |
Solar system in the E-ELT era |
12:30-13:30 | Fabrizio Fiore |
AGN & SN feedback: from galaxy evolution to the reionization epoch era |
13:30-15:00 | Lunch | |
15:00-15:30 |
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Students' talks
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15:30-16:30 | Andrew Shearer |
High time resolution science and technology in the E-ELT era
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16:30-17:30 | Eline Tolstoy |
Resolved stellar populations in the nearby Universe
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17:30-18:00 | Tea Break | |
18:00-19:00 | Maurizio Salaris |
Advanced evolutionary phases current status and open problems |
Day 7, Wednesday, Oct. 14 | ||
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09:00-10:00 | Roberto Tamai |
E-ELT project current status and future plans |
10:00-11:00 | Christoph Keller |
Polarimetry in the E-ELT era |
11:00-11:30 | Coffee Break | |
11:30-12:30 | Marcella Marconi |
Stellar variability in the E-ELT era |
12:30-13:30 | Eline Tolstoy |
Resolved stellar populations in the nearby Universe |
13:30-15:00 | Lunch | |
15:00-15:30 |
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Students' talks
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15:30-16:30 | Markus Kasper |
Extrasolar planets in the E-ELT era
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16:30-17:30 | Bruno Leibundgut |
The VLT Telescope |
17:30-18:00 | Tea Break | |
18:00-19:00 | Simone Esposito |
AO observations at the LBT with LUCI2 |
Day 8, Thursday, Oct. 15 | ||
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09:00-09:30 | Marcella Marconi | Stellar variability in the E-ELT era |
09:30-10:00 | Marconi/Inno | Light-curve templates in the large-surveys era |
10:00-10:30 | Matteo Monelli | Multi-band photometry to identify and characterize stellar variability |
10:30-11:00 | Monelli/Dall'Ora | Time-series photometry and light curves of periodic and transients phenomena |
11:00-11:30 | Coffee Break | |
11:30-12:30 | Christoph Keller |
Polarimetry in the E-ELT era |
12:30-13:30 | Norbert Przybilla |
Sky emission and telluric absorption lines in NIR spectra: principles and application |
13:30 | Half-day Excursion |
Day 10, Saturday, Oct. 17 | ||
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09:00-10:00 | Giuseppe Bono |
Resolved Stellar Populations with E-ELT |
10:00-11:00 | Matteo Monelli |
Building up star formation histories |
11:00-11:30 | Coffee Break | |
11:30-12:30
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Carlos Martins | Fundamental Physics and Cosmology |
12:30-13:30 | Markus Kasper |
Extrasolar planets in the E-ELT era |
13:30-15:30 | Lunch | |
15:30- 16:30 | Maria Bergemann | Atmosphere models the transition from from 1D to 3Ds |
16:30- 17:30 | Student talks |
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17:30-18:00 | Tea Break | |
18:00-19:00 | Michel Dennefeld |
Spectrographs: past present and future |
Day 11, Sunday, Oct. 18 | ||
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09:00-10:00 | Suzanne Ramsay |
Star Formation in the E-ELT era |
10:00-11:00 | Sebastian Kamann |
From the method to science: Kinematics and abundances with integral field spectrographs |
11:00-11:30 | Coffee Break | |
11:30-12:30
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Carlos Martins | Fundamental Physics and Cosmology |
12:30-13:30 | Miwa Goto |
Protoplanetary disks in the E-ELT era |
13:30-15:30 | Lunch | |
15:30- 16:30 | Maria Bergemann
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Atmosphere models the transition from from 1D to 3Ds |
16:30- 17:30 | Richard Ellis |
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16:50-17:20 | Tea Break | |
17:20-18:40 | Santi Cassisi | Building up synthetic color magnitude diagrams |
Day 12, Monday, Oct. 19 | ||
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09:00-10:00 | Richard Ellis
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The high redshift universe in the E-ELT era
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10:00-11:00 | Miwa Goto |
Protoplanetary disks in the E-ELT era |
11:00-11:30 | Coffee Break | |
11:30-12:30
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Giuliana Fiorentino |
Accurate and deep NIR photometry in the E-ELT era |
12:30-13:30 | Miguel Urbaneja-Perez |
Red supergiants in the E-ELT era |
13:30-15:30 | Lunch | |
15:30- 16:30 | Michel Dennefeld | Optical transients and spectroscopic follow-up era |
16:30-17:00 | Tea Break |