euclid ec org meeting euclid france apc 07 08 jan 2016
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Etat davancement de la mission Euclid Y. Mellier IAP & CEA/IRFU/SAp www.euclid-ec.org Meeting Euclid France APC, 07-08 Jan 2016 Euclid Level-0 Science Requirements Sector Euclid Targets Measure the cosmic


  1. Etat d’avancement de la mission Euclid Y. Mellier IAP & CEA/IRFU/SAp www.euclid-ec.org Meeting Euclid France APC, 07-08 Jan 2016

  2. Euclid Level-0 Science Requirements Sector Euclid Targets Measure the cosmic expansion history to better than 10% in redshift bins 0.7 < z < 2 . • Look for deviations from w = − 1, indicating a dynamical dark energy. • Dark Energy Euclid alone to give FoM DE > 400 ( 1-sigma errors on w p , & w a of 0.02 and 0.1 respectively) • Measure the growth index, γ , with a precision better than 0.02 • Measure the growth rate to better than 0.05 in redshift bins between 0.5< z < 2. • Test Gravity Separately constrain the two relativistic potentials Ψ , Φ . • Test the cosmological principle • Detect dark matter halos on a mass scale between 10 8 and >10 15 M Sun • Measure the dark matter mass profiles on cluster and galactic scales • Dark Matter Measure the sum of neutrino masses, the number of neutrino species and the neutrino • hierarchy with an accuracy of a few hundredths of an eV Measure the matter power spectrum on a large range of scales in order to extract values for • the parameters σ 8 and n to a 1-sigma accuracy of 0.01. Initial For extended models, improve constraints on n and α wrt to Planck alone by a factor 2. • Conditions Measure a non-Gaussianity parameter f NL for local-type models with an error less than +/-2. • • DE equation of state: P/ ρ = w , and w(a) = w p + w a (a p -a) • Growth rate of structure formation: f ~ Ω γ ; FoM=1/( Δ w a x Δ w p ) > 400 à ~1% precision on w’s . • Meeting Euclid France APC, 07-08 Jan 2016

  3. The ¡ESA ¡Euclid ¡space ¡mission: ¡EC ¡contribu8ons ¡ ¡ PLM+SVM: 2010-2020 La mission Euclid de l’ESA: objectifs scientifiques VIS imaging: 2010-2020 Soyuz@Kourou ? 2020 ( VIS team) NIR spectro-imaging 2010-2020 (NISP team) Surveys: 2010-2028 (Survey WG) SGS: 2010-2028 SWG: 6 yrs - 15,000 deg 2 Ground data • Commisionning – SV 2019-2028 • Euclid opération: 5.5 yrs:Euclid Wide+Deep • +: SNIa, mu-lens, MW? ~100 PB data processing (EC-SGS team) – Science analyses

  4. The ¡ESA ¡Euclid ¡space ¡mission: ¡EC ¡contribu8ons ¡ ¡ PLM+SVM: 2010-2020 La mission Euclid de l’ESA: objectifs scientifiques VIS imaging: 2010-2020 Soyuz@Kourou ? 2020 ( VIS team) NIR spectro-imaging 2010-2020 (NISP team) Surveys: 2010-2028 (Survey WG) SGS: 2010-2028 SWG: 6 yrs - 15,000 deg 2 Ground data • Commisionning – SV 2019-2028 • Euclid opération: 5.5 yrs:Euclid Wide+Deep • +: SNIa, mu-lens, MW? ~100 PB data processing (EC-SGS team) – Science analyses

  5. ESA Euclid mission • - Total mass satellite : Telescope • 2 200 kg Sun shield (Thales Alenia Space) (Airbus Defence • - Dimensions: and Space) • 4,5 m x 3 m • - Launch: end 2020 by a Soyuz rocket from the Kourou space port • - Euclid placed in L2 • - Survey: 6 years VIS+NISP Scientific Service Module instruments (Euclid (Thales Alenia Space) Consortium)

  6. Euclid Consortium organisation/leads Update Meeting Euclid France APC, 07-08 Jan 2016

  7. Euclid Consortium (Jan 2016 - update) Euclid Consortium Jan 04 2015: • 15 countries • 125 labs • 1274 Full members • 329 FR Full member (26%) • 62 Members at large • 115 « Alumni » Meeting Euclid France APC, 07-08 Jan 2016

  8. Euclid Consortium (Jan 2016 - update) 20 Euclid Consortium Board members Y. Mellier ***G. Meylan leaving in December new Swiss ECB to come E. Girin 7 SWG Coordination Group members M. Berthé Leads the Diversity J. Amiaux Committee R. Scaramella S. Wachter Y. Mellier N. Singsengsouvanh P. Schneider J. Peacock T. Maciaszek A. Zacchei M. Cropper M. Sauvage S. Pottinger A. Ealet K. Jahnke R. Azzolini C. Dabin Meeting Euclid France APC, 07-08 Jan 2016

  9. EC Editorial Board and Publication Groups ( (Jan 2016 - Reminder) Euclid Consortium Editorial Board (ECEB) Euclid Consortium Publication Group (ECPG) L. Guzzo J.-G. Cuby M. Sauvvage P. Schneider, J. Peacock J. Brinchmann M. Cropper (T) P. Fosalba Meeting Euclid France APC, 07-08 Jan 2016

  10. Ground Segment – SDC EC functions (Jan 2016 - reminder) scientific Relation with SWG : community • expression of requirements by SWG & MOC SOC Euclid collaborative work on ESOC ESAC validation External data (PanStarrs, DES, ...) Ground Relation with • DDS EAS Station instruments : provide expertise for the first-rank OUs, place requirements A. Zacchei Simulation on data processing Project Office OU-SIM related to instrument M. Sauvage quality. C. Neisser K. Noddle O. Williams M. Frailis H. Teplitz System Team SDC C. Dabin SDC SDC SDC SDC SDC SDC SDC SDC Relation with ECL • support : survey strategy P. Dubath M. Poncet J. Koppenhofer E. Keihanen impacts data processing, SGS supports the E2E activities. OU-NIR OU-PHZ OU-SHE OU-VIS OU-LE3 OU-SPE OU-SIR OU-MER OU-EXT Nir Imag Phot Red Sh. Morpho & Shear VIS Imag Level 3 Spectro Meas Nir Spectro Euclidisation Ext Data OU coordinator OU Deputy Coordinator Meeting Euclid France APC, 07-08 Jan 2016

  11. Ground Segment – OU EC functions (Jan 2016 - update) EC-SGS functions scientific • Instrument Operation community Teams (IOTs ): maintenance of the instruments, MOC SOC Euclid production of weekly ESOC ESAC instrument reports. External data (PanStarrs, DES, ...) Ground DDS EAS Station • Science Data Centres (SDCs) , host the IOTs and S. Serrano run Processing Functions A. Ealet A. Zacchei Simulation Project Office (pipelines) produced by OU-SIM M. Sauvage Organisational Units System Team (OU s); SDC C. Dabin SDC SDC SDC SDC SDC SDC SDC SDC • SDC’s use Level 1 data T. Kitching J.-L. Starck A.Grazian/ from SOC and produce H. Hoekstra E. Branchini M. Scodeggio G. Polenta Level 2 and 3. Reprocess M. Kilbinger F. Abdalla Y. Copin R. Bouwens external data: Level E. OU-NIR OU-PHZ OU-SHE OU-VIS OU-LE3 OU-SPE OU-SIR OU-MER OU-EXT Nir Imag Phot Red Sh. Morpho & Shear VIS Imag Level 3 Spectro Meas Nir Spectro Euclidisation Ext Data A.Fontana S. Paltani C. Grenet O. Le Fèvre G. Verdoes-Kleijn OU coordinator OU Deputy Coordinator H. Dole F. Castander H. McCracken M. Mignoli J. Mohr M. Kuemmel K. Benson Meeting Euclid France APC, 07-08 Jan 2016

  12. Science Working Groups (Jan 2016 - update) T. Kitching, L. Amendola, J. Brinchmann, W. Percival, H. Hoekstra, L. Guzzo, C. Conselice H. Hoekstra L. Moscardini M. Meneghetti P. Fosalba J. Brinchmann E. Tolstoy J.-P. Beaulieu T. Kitching J. Weller J.-P. Kneib R. Teyssier D. Elbaz A. Ferguson M. Zapatero-Osorio M. Kilbinger J. Bartlett R. Gavazzi A. Cimatti E. Kerins L. Guzzo N. Aghanim L. Amendola J.-G. Cuby B. Poggianti I. Hook W. Percival C. Baccigalupi M. Kunz S. Toft C. Conselice C. Tao Y. Wang M. Viel Position transiens B. Altieri C. Tao (EC) Meeting Euclid France APC, 07-08 Jan 2016

  13. Euclid planning history ¡2011 ¡-­‑ ¡2015 ¡ VIS & NSIP NISP SRR Mission SRR subsystems Board Feb 2014 VIS SRR CDRs begin Phase A Jun-Jul May-Jul BDCR Extension Mission SRR SGS PRR PLM PDR SGS SRR KO IDCR KO Nov 2013 review May 2014 Jan 2015 May-Jul Phase B2 Phase B1 2012 2011 2012 2013 2015 2014 SCS CDR Mar MOC CRR VIS PDR Cal. Review S/C PDR Dec 2011 Apr 2012 Nov 2013 Apr 2014 Sep 2014 May-Jul PLM ITT PLM System PLM SRR System Prime NISP PDR Nov 2013 Mission PDR July 2012 ITT May 2014 Contract Sep-Oct Contract Jul 2013 Adoption Dec 2012 June 2012 MLA Consortium Meeting Euclid France APC, 07-08 Jan 2016

  14. Overview mission timeline and … 2016 Implementation Definition Operations 2024 2012 2016 2020 2008 2028 Proposal selection Mission adoption Launch End nominal mission 2016 Lisbon 2016 EC 2013 2014 2015 2017 Annual Meeting I/PLM SRRs I/PLM PDRs VIS CDR SGS PLM- System-PDR PLM-FM SGS PRR TK1 CDR SGS SRR NISP CDR M-PDR M-SRR AIV start Prime Selection TAS-I Turin Major milestones passed since Lausanne: • System PDR => project is in full C/D Phase • Mission PDR, Board 20 October 2015 • VIS and NISP subsystem CDRs started Meeting Euclid France APC, 07-08 Jan 2016

  15. Launch delayed Meeting Euclid France APC, 07-08 Jan 2016

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