Skip to main content
Go to the home page of the European Commission (opens in new window)
English English
CORDIS - EU research results
CORDIS
Content archived on 2024-06-18

The Physics of the Most Luminous Galaxies

Objective

Exceptionally luminous and active galaxies are cosmic laboratories in which familiar astrophysical processes such as star formation can be studied in extreme environments and under extreme conditions. At the same time, relativistic phenomena, such as mass accretion onto supermassive black holes and launching of relativistic jets, are encountered and can be studied on mass and spatial scales many orders of magnitude higher than their stellar-remnant counterparts. Here, we propose a four-year joint programme between the Astrophysics Group at FORTH in Greece, the Max-Planck Institute for Radioastronomy in Germany, and the California Institute of Technology in the United States, with the aim to strengthen existing collaborations and create a lasting partnership between our institutions for the observational and theoretical study of the astrophysics of all modes of energy release in luminous and active galaxies, including those associated with the central supermassive black hole, and those associated with star formation. To this end, we propose a series of research staff exchanges and networking activities, with the following objectives: (a) strengthen existing collaborations and promote an enhanced effectiveness and productivity in our ongoing efforts; (b) explore further topics of possible collaboration based on the complementarities in the expertise of researchers in our institutions; (c) achieve mutual transfer of knowledge through the training of young researchers, seminars, and workshops; and (d) cement a long-term, sustainable collaboration between our three institutions. Our programme features complementary observational and theoretical parts, and specific tasks involve the radio, optical, and gamma-ray monitoring of blazars, including polarimetric studies; the X-ray studies of active galaxies with the upcoming NuSTAR mission; infrared studies of ultra-luminous galaxies with Herschel; and the theoretical modeling of blazar jets and star-forming regions.

Fields of science (EuroSciVoc)

CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques. See: https://op.europa.eu/en/web/eu-vocabularies/euroscivoc.

You need to log in or register to use this function

Topic(s)

Calls for proposals are divided into topics. A topic defines a specific subject or area for which applicants can submit proposals. The description of a topic comprises its specific scope and the expected impact of the funded project.

Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

FP7-PEOPLE-2012-IRSES
See other projects for this call

Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

MC-IRSES - International research staff exchange scheme (IRSES)

Coordinator

IDRYMA TECHNOLOGIAS KAI EREVNAS
EU contribution
€ 113 000,00
Address
N PLASTIRA STR 100
70 013 IRAKLEIO
Greece

See on map

Region
Νησιά Αιγαίου Κρήτη Ηράκλειο
Activity type
Research Organisations
Links
Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

No data

Participants (1)

My booklet 0 0