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XMM-Newton : a pathfinder for future multi-wavelength and multi-messenger observations with Athena

Project description

New methods to observe the X-ray transient sky

Observing the sky in X-rays allows the detection of the hottest and most energetic phenomena in the universe. Multi-messenger astronomy – the combination of electromagnetic light with gravitational waves and neutrinos – has enabled astronomers to understand the observed X-ray sources. Time-domain astronomy has also helped them study transient sources. The EU-funded XMM2ATHENA project brings together members of the XMM-Newton space observatory and the Athena X-ray observatory to develop new methods and software that should allow researchers to observe the X-ray transient sky in real time and also identify multi-wavelength counterparts of the detected sources and determine their nature using advanced machine-learning methods. Innovative algorithms should allow the probing of hitherto undetected faint sources.

Objective

Observing the sky in X-rays allows us to detect the hottest and most energetic phenomena in the Universe. X-rays allow us to detect matter being accreted onto black holes and they allow us to identify stellar flares from active stars, supernova explosions, neutron stars, white dwarfs, galaxy clusters and even aurora on planets or comets. XMM-Newton, a European Space Agency X-ray observatory has been observing the X-ray, ultra-violet and optical sky for 20 years. However, over this time, astronomy has evolved. We are now rarely looking at individual sources, but populations. We no longer content ourselves to a single wavelength, we are moving towards a multi-wavelength and multi-messenger era where gravitational waves, neutrinos and cosmic rays also help us understand the X-ray sources we observe. We are also moving into an era of time domain astronomy. This means operating our observatories differently. New software and methods need to be put into place to accompany this emerging astronomy, which can then be used by the next generation X-ray observatory, Athena.

This proposal brings together members of the XMM-Newton Science ground segment, key members of the Athena Science ground segment, and other members of the X-ray community with complimentary skills to develop and test new methods and software to allow the community to follow the X-ray transient sky in quasi-real time, identify multi-wavelength/messenger counterparts of the sources detected with XMM-Newton and determine their nature using advanced machine learning methods and probe the faintest sources, hitherto undetected, using innovative stacking and detection algorithms. These methods will then be integrated into the Athena software, currently at the beginning of the developmental phase and the newly detected/identified sources will enhance our preparation of the X-ray sky that will be observed with Athena.

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Topic(s)

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Funding Scheme

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RIA - Research and Innovation action

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Call for proposal

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(opens in new window) H2020-SPACE-2018-2020

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Coordinator

CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 502 648,75
Address
RUE MICHEL ANGE 3
75794 PARIS
France

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Region
Ile-de-France Ile-de-France Hauts-de-Seine
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.

€ 657 973,75

Participants (10)

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