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Content archived on 2024-06-18

Probing Strong Gravity by Black Holes Across the Range of Masses

Objective

Black holes provide a crucial link between Einstein’s theory of gravity and real cosmic objects which astronomers can observe and study in the Universe. This project is oriented towards legacy of the cornerstone XMM-Newton X-ray satellite mission of European Space Agency (ESA) in synergy with relevant data in other spectral domains that are covered by ground-based infrared and radio interferometric techniques at European Southern Observatory (ESO) and elsewhere. Information in different wavelengths will be gathered and explored in order to understand radiation processes in places of strong gravity, near black holes. We will address outstanding questions of determining the black hole spin, measuring the location of the accretion disc inner rim, and revealing connections between inflows and outflows in these objects. To this end we will analyze and interpret multi-wavelength spectral and fast timing information on accreting black holes in compact binaries, in cores of active galactic nuclei, as well as other galaxies exhibiting low level of activity due to intermittent supply of gas from the cosmic environment or by switching to a radiatively inefficient regime. We will include valuable data from archives and complement them by performing new observations where needed. Our main objective is to use and enhance computational tools that the participating groups have been developing over two decades, and to join our effort in a dedicated program of data analysis and science interpretation of the most bizarre cosmic objects. We will rely on unprecedented combination of sensitivity and energy resolution of current X-ray missions of ESA, together with wide spectral coverage by ground-based observatories in ESO and elsewhere. The developed techniques will be highly relevant in the context of new missions. We will make our tools available to the entire scientific community. The research team includes experts from 7 leading research institutes and universities.

Fields of science (EuroSciVoc)

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Programme(s)

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Topic(s)

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Call for proposal

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FP7-SPACE-2012-1
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.

CP-FP - Small or medium-scale focused research project

Coordinator

ASTRONOMICKY USTAV AV CR
EU contribution
€ 352 352,00
Address
FRICOVA 298
25165 Ondrejov
Czechia

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Region
Česko Střední Čechy Středočeský kraj
Activity type
Research Organisations
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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.

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Participants (6)

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