Monday, July 1
09:00 - 10:00	Registration and coffee
10:00 - 10:10	Opening session
SESSION 1: Present Observational Status
	Space and Ground Based Data
10:10 - 10:40	'Space and ground based data for Asteroseismology' - H. Kjeldsen, Aarhus Universitet, Denmark
	Present Status for Different Pulsators
10:40 - 11:00	'Present Observational Status of Solar-type stars' - F. Bouchy, Observatoire de Geneve, Switzerland
11:00 - 11:20	'Present Observational Status of the Intermediate Mass Stars: Sct stars, Dor stars and roAp stars' - Don Kurtz, University of Central Lancashire, U.K.
11:20 - 11:40	'Present observational status of high mass pulsating stars' - P. De Cat, University of Leuven, Belgium
11:40 - 12:00	'Advanced post-main Sequence stars' - S. O'Brien, Space Telescope Science Institute, USA
12:00 - 14:00	Lunch
14:00 - 14:20	' Scuti pulsations in intermediate mass pre-main sequence stars' - C. Catala, Observatoire de Paris, France
14:20 - 14:35	'Discovery of A New Class of Pulsating Stars: Gravity-mode Pulsators among Subdwarf B Stars' - E.M. Green, Steward Observatory, USA
14:35 - 14:50	'STARE results on a single field: tens of new pulsating stars' - R. Alonso, Instituto de Astrofísica de Canarias, Spain
	The Sun as a Star
14:50 - 15:10	'The sun as a star' - P. Palle, Institute de Astrofisica de Canarias, Spain
15:10 - 16:00	Tea break
SESSION 2: Asteroseismic Techniques
	Mode Identification and Frequency Determination
16:00 - 16:30	'Multicolour photometry for mode identification' - M. Reed, Southwest Missouri State University, USA
16:30 - 17:00	'High-resolution spectroscopy for mode identification' - J. Telting, Nordic Optical Telescope, Spain
17:00 - 17:15	'Mode identification from line profiles using the direct fitting technique' - L.A. Balona, South African Astronomical Observatory, South Africa
17:15 - 17:30	'Revisiting the Moment Method as a Mode Identification Technique' - J. De Ridder, Institute of Astronomy Leuver, Belgium
17:30 - 17:45	'An improved photometric mode identification method: applications to Slowly Pulsating B stars, Cephei, Scuti and Doradus stars.' - M.A. Dupret, Université de Liège, Belgium
19:30	Welcome Reception - Centro de Astrofísica da Universidade do Porto
Tuesday, July 2
09:30 - 10:00	'Theoretical clues for mode identification - instability ranges and rotational splitting patterns' - A. Pamyatnykh, Copernicus Astronomical Center, Poland
10:00 - 10:30	'Peakbagging for solar-like stars' - T. Appourchaux, ESA, Holand
10:30 - 11:15	Coffee Break
11:15 - 11:30	'Photometric nonadiabatic observables in rotating Cephei models ' - J. Daszynska-Daszkiewicz, Astronomical Institute of the Wroclaw University, Poland
11:30 - 11:45	' Solar-like oscillations in red giants ' -T.R. Bedding University of Sydney , Australia
11:45 - 12:00	'Are gravity modes found in –Scuti stars?' - M. Breger, Institute of Astronomy, University of Vienna, Austria
12:00 - 14:00	Lunch
14:00 - 14:15	'A new approach to the multiperiodic analysis of massive time series' - M.Bossi, NAF - Osservatorio Astronomico di Brera, Italy
	Inferring Information from the Frequencies
14:15 - 14:45	'Seismic inference using Monte Carlo explorations of model space' - T. Metcalfe, Aarhus Universitet, Denmark
14:45 - 15:15	'Stellar inversions' - S. Basu, Yale University, USA
15:15 - 16:00	Tea break
16:00 - 16:30	'Asteroseismic inference' - D. Gough, Cambridge University, U.K.
16:30 - 16:45	'Inversions for the internal structure of stars using the differential response technique' - I.W. Roxburgh, Queen Mary University of London, U.K.
16:45 - 17:00	'p-mode oscillations of -Cen A: the need for space asteroseismology' - A.Thoul, Université de Liege, Belgium
17:30	Porto City Tour (optional - see details)
Wednsday, July 3
09:00 - 20:00	Douro Vintage Programme (optional - see details)
Thursday, July 4
SESSION 3: Asteroseismic Constraints on Stellar Structure and Evolution
	Solar-like and near-main sequence stars
09:30 - 10:00	'Stellar convection' - P. Demarque, Yale University, U.S.A.
10:00 - 10:30	'Stellar Rotation and Internal Angular Momentum Transport' - M. Pinsonneault, Ohio State University, U.S.A.
10:30 - 11:30	Coffee break
11:30 - 11:45	'Are pulsation and magnetic axes aligned in roAp stars?' - L. Bigot, Niels Borh Institute - Astronomical Observatory, Denmark
11:45 - 12:00	'Seismic diagnostics on stellar convection treatment from oscillation amplitudes of p-modes ' - M.J. Goupil, Observatoire de Paris, Meudon, France
12:00 - 14:00	Lunch
14:00 - 14:30	'Mixing and diffusion in stars' - S. Vauclair, Observatoire Midi Pyrénées, France
14:30 - 14:45	'Of Variability, or its Absence, in HgMn stars' - S. Turcotte, Lawrence Livermore National Laboratory, USA
14:45 - 15:00	'A study of the solar-like properties of -Hydri' - M.P. Di Mauro , INAF-Osservatorio Astrofisico di Catania, Italy
15:00 - 15:15	'Giant vibrations in dip' - T.C. Teixeira, Centro de Astrofísica da Universidade do Porto, Portugal
15:15 - 15:30	'Stochastic excitation of gravity waves by overshooting convection in solar-type stars' - B. Dintrans, Observatoire Midi-Pyrénées, France
15:30 - 16:20	Tea break
	Away from the main sequence (childhood and old age)
16:20 - 16:50	'Outstanding issues for post-main sequence evolution' - G. Fontaine, University of Montreal, Canada
16:50 - 17:05	'Hot Subdwarfs: magnetic, oscillatory and other physical properties ' - A. Ulla, Universidade de Vigo, Spain
17:05 - 17:20	'Nonlinearity of nonradial modes in evolved stars' - R.M. Nowakowski, Copernicus Astronomical Center, Poland
19:00	Conference Banquet
Friday, July 5
09:30 - 10:00	'Outstanding Issues for Pre-Main Sequence Evolution' - F. Palla, Observatorio de Arcetri, Italy
10:00 - 10:15	'New observational results on PMS Scuti stars' - V. Ripepi, Osservatorio Astronomico di Capodimonte, Italy
10:15 - 10:30	'PMS -Scuti stars: theory versus observations' - M. Marconi, Osservatorio Astronomico di Capodimonte, Italy
10:30 - 10:35	'The Eddington Mission' - I.W. Roxburgh, Queen Mary University of London, U.K.
10:35 - 11:15	Coffee break
SESSION 4: Closing Section
11:15 - 12:00	'Summary: problems, connections and expectations' - J. Christensen-Dalsgaard, Aarhus Universitet, Denmark