Invited talks
Nikos Prantzos (France): Why we need to map oxygen in the Universe
Sylvia Ekstrom (Switzerland): How well do we know oxygen yields from massive stars?
Amanda Karakas (Australia): Oxygen production on the AGB and the relevance of planetary nebulae to map the oxygen abundance in galaxies
Martin Asplund (Germany): The solar oxygen abundance : a new standard
Héctor Socas-Navarro (Spain): Alternative determinations of the solar oxygen abundance
Katharina Lodders (US): Constraints on the solar oxygen abundance from meteorites, planets, and other planetary objects
Iván Ramirez (US): Oxygen abundance determinations in solar-type stars
Sergei Andrievsky (Ukraine): Oxygen abundance determinations in cool giant stars
Norbert Przybilla (Germany): Oxygen abundance determinations in A-supergiants
Miguel A. Urbaneja (US): Oxygen abundance determinations in OB dwarfs and supergiants
Mónica Rodríguez (Mexico): Temperature-based oxygen abundances in HII regions and PNe
Christophe Morisset (Mexico): Oxygen abundances in ionized nebulae from photoionization model-fitting
Antonio Peimbert (Mexico): Temperature fluctuations in ionized nebulae and their effect on the oxygen abundance determination
Lisa Kewley (US): Strong-line methods for oxygen abundance determinations in giant HII regions and emission line galaxies
Roberto Maiolino (Italy): Oxygen abundance determination at high redshift from emission lines
Edward Jenkins (US): The oxygen abundance in the local ISM from absorption lines
Miroslava Dessauges-Zavadzky (Switzerland): The oxygen abundances at high redshift from absorption lines
Kyoko Matsushita (Japan): The oxygen abundance from X-rays: methods and prospects
Claudio Mendoza (Venezuela): The reliability of atomic data used for oxygen abundance determinations
Lars Mattsson (Denmark): Oxygen-rich dust production in the atmospheres of cool stars and in supernovae
Anthony Jones (France): Oxygen-rich dust processing and evolution in the interstellar medium
William Henney (Mexico): Is oxygen well-mixed in the sites where it is observed?
