1. ESA UNCLASSIFIED – For Official Use News from the Archives Guido De Marchi & Bruno Merín 13/05/2015 - ESTEC

2. ESDC organisational structure Astro Archives Science Lead XSA KP HSA KP PLA KP CSA KP EAS KPGACS KP HST KP LPF KP MEX, VEX Rosetta KP Exomars KP BACS KP SolO KP Ulysses Soho Planetary Archives Science Lead Solar Helio Archives Science Lead ISO Exosat Astro Archives Technical Lead Solar Helio Archives Tech. Lead Planetary Archives Technical Lead Astro Archive Group PSA Group PSA KP (Huygens, Giotto) Solar Helio Archive Group Group of archive software developers common software libraries and tools repository, full open source H/SRE-OE KP: Key Person Important note: individual boxes correspond to roles, not necessarily to a full time position Astro SOCs/SGSs Planetary SOCs/SGSs Solar Helio SOCs/SGSs Archives Head Scientist MMI KP (acting)

3. Names and roles of leads Bruno MerínAstronomy science lead Jesus SalgadoAstronomy technical lead Guido De MarchiHead scientist Planetary science lead (acting) Isa BarbarisiPlanetary technical lead Arnaud MassonHeliophysics science lead Beatriz MartinezHeliophysics technical lead (acting)

4. Role of Archives Science Leads 1.Science Leader of archives in their domain a.Coordination of individual missions Archive Scientists b.Science guidelines for archives long term preservation c.ESA science presence at “virtual observatory”-type initiatives d.Science Leader of multi-mission initiatives in their domain 2.Daily interactions with Technical Lead and SW developers a.In coordination with Archive Scientists, DM/MM, PS, Head Scientist: adapt tasks priority within Group of archive SW developers 3.Does Science with archives 4.Organize archives “science” Reviews 5.Outreach: newsletters, usage stats and publications report, science conferences, …

5. Role of Archives Chief Scientist 1.Chief Scientist with overall scientific guidance for all ESA Science Archives a.Overarching view on all disciplines archives b.Common theme and vision for all archives 2.Major role of communication and science support in several directions a.Close interactions with Project Scientists, based at ESTEC b.With missions Archive Scientists c.Provide independent oversight to H/SRE-OE, H/SRE-OO, H/SRE-OD d.With Astro/Planetary/Solar Helio Archives Science Leads e.With ESTEC/ESAC Faculties 3.Does science through archive data exploitation 4.Participate to Archives review, outreach activities 5.Provide overall archival scientific guidance, with potential negotiation priorities between archives when decisions are needed

6. The Multi-Mission Interface 1.Goal: to facilitate data discovery and archival science for ALL users a.Multi-wavelength b.Project agnostic c.Exploration

7. The Multi-Mission Interface 1.Goal: to facilitate data discovery and archival science for ALL users a.Multi-wavelength b.Project agnostic c.Exploration 2.Interface to all astronomy archives 3.Current status is a first prototype Multi-mission interface Herschel XMM- Newton HSTPlanckISOIntegralEXOSATFuture..

8. The Multi-Mission Interface prototype 1.Ingredients of first prototype: a.Access to data in individual archives b.All-sky (aka HiPS) c.Footprints 2.Use cases of first prototype: a.Explore multi-wavelength skies b.Single and multiple targets 3.Images and catalogues only, selected mission

9. MMI Prototype: URL, video and feedback MMI protoype URL (do not disclose): http://ammi.esac.esa.int/ Video of MMI demo: http://youtu.be/7cyXGP-K_GA Feedback : http://mmi-forum.wikispaces.com/home