About EGO

Who we are

Who we are

Governance

Departments

History

People

Who we are

EGO – the European Gravitational Observatory – is located in the countryside near Pisa in the Commune of Cascina.

In order to ensure the long term scientific exploitation of the VIRGO interferometric antenna for gravitational waves detection as well as to foster European collaboration in this upcoming field, the VIRGO funding institutions (CNRS for France and INFN for Italy) have created a consortium called EGO (European Gravitational Observatory).

VIRGO is a 3-km long interferometer built in the framework of a French-Italian collaboration. Today, this collaboration involves 19 laboratories with more than 250 scientists in France, Italy and also in the Netherlands, Poland and Hungary as well.

EGO pursues these main objectives:

  • ensure the commissioning of the VIRGO antenna for gravitational waves, its operation, maintenance and upgrades;
  • create and run a computing centre for the data analysis;
  • ensure the maintenance of the site and its related infrastructures;
  • promote R&D activities useful for the detection of gravitational waves;
  • carry out any other research in the field of gravitation of common interest to the Members;
  • promote co-operation in the field of the experimental and theoretical gravitational waves research in Europe;
  • promote contacts among scientists and engineers, the dissemination of information and the advanced training of young researchers.

Gravitational waves detection will open a totally new window in the observation of the Universe and in the understanding of its origin and evolution. The gravitational waves observation window is complementary to other windows of observation already available with other cosmic radiation. These are represented by the observation of light and the other electromagnetic waves that are emitted by stars, galaxies and other celestial bodies and by the detection of cosmic ray particles.

A collaboration was set up to design and then build a world-class interferometer, called VIRGO, with two 3 km-long perpendicular arms, to detect and measure gravitational waves. The VIRGO collaboration is the result of a French-Italian co-operative effort among 19 laboratories and institutes. When finally commissioned, it is expected that VIRGO’s sensitivity will be capable of measuring strains that are smaller than the dimension of an atom with respect to the distance between the Earth and the Sun. The funding institutions of the VIRGO collaboration (CNRS – Centre National de la Recherche Scientifique – for France, and INFN – Istituto Nazionale di Fisica Nucleare – for Italy) decided in December 2000 the creation of EGO. They established EGO as a consortium between themselves, operating under the Italian law within the legal framework of a private company. Once completed the construction of the interferometer in 2003, VIRGO started the commissioning phase. In 2007, after approaching the design sensitivity in a major part of the accessible frequency range, VIRGO performed its first scientific data taking run, lasting from May 18 to October first. Today a two step (“VIRGO+” and “Advanced VIRGO”) upgrade/data-taking program is ongoing, in order to improve the sensitivity by 10 times within 2013. Reaching this goal will increase by 1000 times the volume of explored universe and by the same factor the gravitational wave detection probability. At that time scientists are confident that probability will turn into certitude. EGO has been given the mission to ensure the long term scientific exploitation of VIRGO as well as to foster European collaboration in the field of gravitational waves observation. EGO is providing VIRGO with the supporting infrastructure, including buildings, networks, computing facilities, administration, general services, maintenance as well as support for the interferometer operation and upgrade. EGO is open to the participation of institutions from other European countries as well to the collaboration in the field of gravitational waves research with institutions and laboratories worldwide. EGO with VIRGO is located in the territory of Cascina, a small town a few kilometres from Pisa, in grounds belonging to INFN. The governing body of EGO is the Council, the members of which are nominated by the funding institutions. The Scientific and Technical Advisory Committee (STAC), advises the Council on scientific and technical activities carried out by the Consortium.

EGO welcomes you to its web site, where you will find details about its location and its organisation as well as useful links to the Virgo web pages and to relevant information about gravitational waves and their detectors.

EGO COUNCIL

EGO Council

EGO is established under the Italian law. Its governing body is the Council composed of members nominated by the funding institutions. The Council appoints a Director who is the legal representative and chief executive of EGO.

The Council is the decision-making body of the EGO consortium. The Director of EGO is responsible to carry on and execute the Council decisions. The Council and the Director of EGO operate according to EGO statute.

The Council is composed by three representatives of CNRS and three representatives of INFN, among which is elected the President. The Council usually meets twice a year. The Director of EGO participates in the Council meetings but has no right to vote. Observers may be nominated by the Council Members CNRS and INFN and invited persons may participate for discussing specific items of the agenda.

At present the Council is composed as follows:

For CNRS
Berrie Giebels, Vice-President
Guy Perrin
Thérèse Huet
For INFN
Antonio Masiero, President
Marco Grassi
Marco Pallavicini
For Nikhef
Stan Bentvelsen
As Council Advisor
Veronica Bucchieri
Roberto Pellegrini

Scientific & Technical Advisory Committee

According to the dispositions of the Statute of the EGO Consortium, the EGO Council sets up a Scientific and Technical Advisory Committee (STAC), composed of up to ten scientific personalities. It also appoints the chairperson of the STAC.

The role of the STAC is to advice the EGO Council.

For this purpose, the STAC meets on the site of the EGO Consortium at least twice per year, to follow and assess the progress on the scientific and technical activities carried on.

The STAC chairperson appointed for three years presents the outcome of the meetings to the EGO Council.

For more details on the STAC duties, consult the Terms of reference of the STAC.

The present composition of the STAC is the following:

  • David Shoemaker, Chairman (MIT LIGO Lab.)
  • Gerhard Heinzel, Vice-Chairman (AEI Hannover)
  • Dominique Boutigny (CNRS-LAPP)
  • Rita Dolesi (University of Trento)
  • Andreas Freise (University of Birmingham)
  • Giuseppe Ruoso (INFN Legnaro)
  • B.S. Sathyaprakash (Cardiff School of Physics & Astronomy)
  • Stephen Smartt (Queen’s University Belfast)
  • Takayuki Tomaru (NAOJ)
  • Peter Wolf (Observatoire de Paris)

The EGO directorate secretariat helps the STAC in organising its meetings.

Our Structure

Our Structure

For Technological and Administration responsibilities EGO’s Director is assisted by the Technical Deputy Director, the Administrative Deputy Director and by five Heads Department, who respectively manage:

Administration, Budget management for EGO including upgrade projects of VIRGO interferometer, Human Ressources and European projects of which EGO is the leader or co-manager from the European Commission.

Information Technology department manages the computing, storage and network systems at the EGO site providing the IT infrastructure for the control of the Virgo Interferometer, the running of the on-line data analysis and the data exchange with the external computing centers and the other detectors, working actively in the software development for many subsystems.

Interferometer Technology, In charge of operations maintenance, participates of upgrade and running operation of VIRGO interferometer. The ITF department is based on tree main expertises Optics benches and injection beam light, Electronics low noise and Environment Noise analysis and mitigation.

General Infrastructure, Management of all infrastructure facilities, services, supplies needs and all EGO site buildings and facilities for VIRGO interferometer running needs.

Vacuum & Mechanics, Management of operation, maintenance and upgrades of the Virgo Vacuum System and provides support for mechanical design and on-site workshop capability.

For any question or first contact concerning Technological and Administrative Departments send an email to: EGO Departments Contact Form

Organizational charts of EGO

Our History

Our History

We are working on this page…

Picture: INFN, Simone Schiavon

 

Our People

Our People

We are working on this page…

Picture: INFN, Simone Schiavon