Presentation of the first data release from Gaia mission at UB

A public ceremony will take place at Phyisics Faculty of the Universitat de Barcelona on the occasion of the First Gaia Data Release on 14th September 2016, and guided visits to the exhibition "Mil milions d'ulls per a mil milions d'estrelles".

ESA's billion-star surveyor Gaia, was launched on 19 December 2013, and it is in routine science operations since 25 July 2014. Data released corespond to the observations of the first 14th months of the mision.


Date:14 September

Place: Aula Magna Enric Casassas (Physics Faculty)


11:45 : Presentation (Dra. Francesca Figueras)

11:50 : The two first years of the Gaia mission (Dra. Mercè Romero-Gómez)

12:00 : Barcelona’s participation in Gaia (Dr. Jordi Portell)

12:10 : The first data release from Gaia (Dr. Josep Manel Carrasco)

12:20 : Connexion to ESAC event webstreaming to the official archive opening (Dra. Carme Jordi)

12:30 : Questions and Answers

12:45 : End, First 3D images of the Solar Neighbourhood


Note: attention to the media 11:15

Guided visits to the exhibition Mil milions d'ulls per a mil milions d'estrelles

Date: 15 and 16 September 2016

Place:  Physics Faculty Hall

Adressed to degree and master students

Timetable: from 10:20 to 10:45; from 16:50 to 17:10

Inscription at the faculty secretary office


Gaia Mission

Gaia is designed to map more than 1 billion stars in our Galaxy, and to provide positions, parallaxes and proper motions at an unprecedented accuracy level, far below a milliarcsecond. These accuracies can only be achieved after a complex data processing that requires observations taken throughout the 5-year nominal mission. For this reason, the final Gaia results will not be available until the early 2020s, but a number of early releases have been foreseen, based on increasingly longer stretches of observations.

First Data Release

The first Gaia data release, which will be available online on 14 September, will include the positions and G magnitude for about one billion stars using observations taken between 25 July 2014 and 16 September 2015.

In addition, for a subset of data – about 2 million stars in common between the Tycho-2 Catalogue and Gaia – there will be a five-parameter astrometric solution, giving the positions, parallaxes, and proper motions for those objects. This is referred to as the Tycho-Gaia Astrometric Solution (TGAS).

Photometric data for RR Lyrae and Cepheid variable stars that were observed frequently during a special scanning mode that repeatedly covered the ecliptic poles will also be made public.

ICCUB participation in the Gaia mission

The Gaia UB team is composed by researchers from the Institute of Cosmos Sciences of the University of Barcelona (ICCUB), the Institute of Space Studies of Catalonia (IEEC). The team has been involved in the Gaia mission since the very early phases. It has played a major role in the scientific and technological design of the instrumentation, database prototypes and data simulation. It has also developed a calibration algorithm of photometric data, and the system that will enable to daily process satellite’s data and store them in a database to later extract the first scientific results.


Furthermore, the group is developing tools for scientific exploitation, by means of data got from the Earth in order to complement those provided by Gaia. The Data Processing Center of Barcelona, which includes CESCA and the Barcelona Supercomputer Center, provides resources to carry out some operations throughout the mission and has been a necessary tool to carry out simulations in order to test the instrument.


Gaia UB Group

Gaia on the ESA website




Miércoles, 14 Septiembre, 2016