Common Data Centre Infrastructure for Astronomy, Astropar cle and Cosmology (CDCI) Andrii Neronov (UNIGE) Space astronomical data landscape at the Astronomy Department (DA) of UNIGE
POLAR
Ground segment Ground segment Ground segment
Science data Centre Contribu on to the Data processing centre data analysis pipeline
Scien fic leadership is the key point for the successful ground segment / data centre ac vi es: – data analysis algorithms are ini ally developed / tested by scien sts who are mo vated to extract most of the observa onal data – the algorithms are incorporated into consistent data analysis framework by scien sts + so ware engineers – the framework is validated and con nuously improved through the feedback of scien fic community exploi ng the data
Opera on of the science data centre provides “proximity” of the data favouring a wide range of high impact science results and good visibility in astronomical and broad scien fic community. Space astronomical data landscape at the Astronomy Department (DA) of UNIGE
INTEGRAL Planck GAIA
POLAR
Past / ongoing
Future Athena
Science Data Centre Data processing centre Science Opera ons Centre Ground segment Ground segment Ground segment Science data Centre EUCLID CHEOPS
Data Centre / ground segment ac vi es for missions in prepara on profit from previous development. Projects could profit from “cross-breeding”. Space astronomical data landscape at the Astronomy Department (DA) of UNIGE
INTEGRAL Planck microwave GAIA Hard X-ray / gamma-ray
POLAR
visible
Hard X-ray /gamma-ray visible Athena
visible X-ray
EUCLID CHEOPS
Ground segment / data centre development exper se could be successfully extended across different domains of electromagne c spectrum. Space / ground-based astronomical data landscape at the Astronomy Department (DA) of UNIGE
INTEGRAL Planck microwave GAIA Hard X-ray / gamma-ray
POLAR
visible
Hard X-ray /gamma-ray visible Athena
visible X-ray EUCLID CHEOPS
very-high-energy gamma-ray radio
Ground segment / data centre development exper se could be extended to ground-based observatories. CTA SKA Space / ground-based astronomical data landscape at the Astronomy Department (DA) of UNIGE, LASTRO (EPFL) Par cle and Nuclear Physics Department (DPNC) Theore cal Physics Department (DPT) INTEGRAL Planck microwave GAIA (DA+DPT) Hard X-ray / gamma-ray
POLAR (DA+DPNC)
visible
Hard X-ray /gamma-ray visible Athena
visible X-ray EUCLID (DA+DPT) (UNIGE+EPFL) CHEOPS
very-high-energy gamma-ray radio
CTA (DA+DPNC) SKA (UNIGE+EPFL) Space / ground-based astronomy / astropar cle data landscape at the Astronomy Department (DA) of UNIGE, LASTRO (EPFL) Par cle and Nuclear Physics Department (DPNC) Theore cal Physics Department (DPT) INTEGRAL Planck microwave GAIA (DA+DPT) Hard X-ray / gamma-ray
POLAR (DA+DPNC)
visible
Hard X-ray /gamma-ray visible Athena
visible X-ray EUCLID (DA+DPT) CHEOPS
very-high-energy gamma-ray HERD EUSO radio
gamma-ray/ cosmic ray
CTA (DA+DPNC) SKA Astronomy / cosmology /astropar cle physics landscape at the Astronomy Department (DA) of UNIGE, LASTRO (EPFL) Par cle and Nuclear Physics Department (DPNC) Theore cal Physics Department (DPT) INTEGRAL Planck GAIA
POLAR Astronomy Cosmology Astronomy
Astronomy Athena
Astronomy/ Cosmology Astronomy Astronomy/ EUCLID (DA+DPT) CHEOPS Cosmology
EUSO Astronomy/ HERD Astropar cle physics Astronomy/ Astropar cle physics Astronomy/ Ground segment / data centre development exper se could be extended to Cosmology CTA A range of astronomy / cosmology / astropar cle physics projects. SKA Astronomy / cosmology /astropar cle physics landscape at the Astronomy Department (DA) of UNIGE, LASTRO (EPFL) Par cle and Nuclear Physics Department (DPNC) Theore cal Physics Department (DPT) INTEGRAL Planck GAIA
POLAR Added value to the data due to the Astronomy Mul -wavelength / mul -messenger Cosmology Astronomy aspect
Astronomy Athena
Astronomy/ Cosmology Astronomy Astronomy/ EUCLID (DA+DPT) CHEOPS Cosmology
EUSO Astronomy/ HERD Astropar cle physics Astronomy/ Astropar cle physics Astronomy/ Ground segment / data centre development exper se could be extended to Cosmology CTA A range of astronomy / cosmology / astropar cle physics projects. SKA Common Data Centre Infrastructure for Astronomy, Astropar cle and Cosmology
Astronomy UNIGE INTEGRAL and/or SSO CDCI Planck GAIA
PI PI PI PI PI PI PI PI PI PI Project scientist PM PM PM PM PM PM PM PM PM System POLAR INTEGRAL GAIA EUCLID CTA
Administration DAMPE Storage Storage Storage Storage Astro Storage CPU Data CPU CPU CPU CPU Bank
Common infrastructure CHEOPS PLATO POLAR HERD Storage Storage Storage Storage CPU CPU CPU Mul -wavelength / mul - CPU Athena messenger data analysis system Astronomy Physics Coherent infrastructure for development and opera on of science data centre(s): – support for future data centre / ground segment projects in the domains of astronomy, EUCLID (DA+DPT) astropar cle physics and cosmology; CHEOPS – long-term preserva on of astronomical data and data analysis tools of past missions / projects; – mul -mission / mul -wavelength / mul -messenger HERD astronomical data archives / public data EUSO access / data analysis system; – reusability of public data sets / reproducibility of scien fic results. Proposal for the Swiss Roadmap for Research Infrastructures for 2017-2020: – reviewed with the highest grade; – recommended for implementa on in 2017-2020 period. CTA SKA Common Data Centre Infrastructure for Astronomy, Astropar cle and Cosmology
INTEGRAL Planck GAIA Microwaves: fluctua ons of cosmic Visible light: Mo on of stars in the microwave background measure the Milky Way allow to measure the Dark Dark Ma er and Dark Energy in the Ma er content of the local Galaxy POLAR X-rays are used to pinpoint the Universe 13 billion years ago. new par cles forming the Dark Ma er
Athena
Visible light: distribu on of galaxies measures the Dark Ma er and Dark Energy in the Universe today / yesterday. X-rays trace the Dark Ma er in galaxy clusters forming today. EUCLID (DA+DPT) CHEOPS
HERD EUSO
Cosmic rays, gamma-rays and neutrinos are used to pinpoint the new par cles forming the Dark Ma er Radio waves from galaxies trace Dark Ma er and Dark Energy back Gamma-rays are used to pinpoint the at the moment of galaxy forma on. new par cles forming the Dark Ma er CTA SKA Common Data Centre Infrastructure for Astronomy, Astropar cle and Cosmology
Astronomy UNIGE INTEGRAL and/or SSO CDCI Planck GAIA
PI PI PI PI PI PI PI PI PI PI
Project scientistPOLAR PM PM PM PM PM PM PM PM PM System INTEGRAL GAIA EUCLID CTA
Administration DAMPE Storage Storage Storage Storage Storage Astro CPU Data CPU CPU CPU CPU Bank
Common infrastructure CHEOPS PLATO POLAR HERD Storage Storage Storage Storage CPU CPU CPU Mul -wavelength / mul - CPU Athena messenger data analysis system Astronomy Physics Coherent infrastructure for development and opera on of science data centre(s): – support for future data centre / ground segment projects in the domains of astronomy, EUCLID (DA+DPT) astropar cle physics and cosmology; CHEOPS – long-term preserva on of astronomical data and data analysis tools of past missions / projects; HERD EUSO – mul -mission / mul -wavelength / mul -messenger astronomical data archives / public data access / data analysis system; – reusability of public data sets / reproducibility of scien fic results. Proposal for the Swiss Roadmap for Research Infrastructures for 2017-2020: – reviewed with the highest grade; – recommended for implementa on in 2017-2020 period. CTA SKA Common Data Centre Infrastructure for Astronomy, Astropar cle and Cosmology
INTEGRAL Planck GAIA
POLAR
~10-30 TB ~50 TB … 600 TB Past / ongoing
Future Athena mul -PB 500 TB
EUCLID (DA+DPT) CHEOPS
HERD EUSO
mul -10 PB 100 PB (?) CTA SKA Common Data Centre Infrastructure for Astronomy, Astropar cle and Cosmology
INTEGRAL Planck GAIA
POLAR
~10-20 TB (compressed) ~50 TB Past / ongoing General public Future Scientists users Athena mul -PB Scientists users Scientists users Scientists users Scientists users Scientists users CDCI 500 TB (UNIGE) EUCLID GAIA INTEGRAL CTA Astro Data Bank other data services: SIMBAD, NED, EUCLID (DA+DPT) CHEOPS HEASARC, ...
HERD EUSO AstroCloud IDSS (EPFL) Common / shared compu ng? Storage Storage Storage Storage CPU CPU CPU CPU
Storage
CPU
mul -10 PB EPFL+UNIGE+SNSC+ EOSC+.... 100 PB (?) CTA SKA Common Data Centre Infrastructure for Astronomy, Astropar cle and Cosmology Coherent infrastructure for development and opera on of science data centre(s): – support for future data centre / ground segment projects in the domains of astronomy, astropar cle physics and cosmology; – long-term preserva on of astronomical data and data analysis tools of past missions / projects; – mul -mission / mul -wavelength / mul -messenger astronomical data archives / public data access / data analysis system; – reusability of public data sets / reproducibility of scien fic results. Proposal for the Swiss Roadmap for Research Infrastructures for 2017-2020: – reviewed with the highest grade; – recommended for implementa on in 2017-2020 period.
Scien fic leadership is the key point for the successful data centre ac vi es: – data analysis algorithms are ini ally developed / tested by scien sts who are mo vated to extract most of the observa onal data – the algorithms are incorporated into consistent data analysis framework by scien sts + so ware engineers – the framework is validated and con nuously improved through the feedback of scien fic community exploi ng the data
Opera on of the science data centre provides “proximity” of the data favouring a wide range of high impact science results and good visibility in astronomical and broad scien fic community.
Data Centre / ground segment ac vi es for missions in prepara on profit from previous development. Projects could profit from “cross-breeding”.