Bandi ESA Intended Invitaon To Tender (ITT): disamina di ... · Bandi ESA Intended Invitaon To...

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INAFHeadquarter,6-Aprile-2017!

ClaudioMacculi

BandiESAIntendedInvita#onToTender(ITT):disaminadiuncaso.

INAFSedeCentrale,6-Aprile-2017

AREMBES:ATHENARadia;onEnvironmentModelsandx-rayBackgroundEffectsSimulators

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Outline

2!

•  HowESAprogrammesaredivided:CTPvsTRL•  RequestforaTDA•  EMITSwebsite: -Howisitstructured? -Docstobedownloaded -Timing

•  InfoontheAREMBESproposal/project -scien;ficcontext -management/planning -products

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ESAProgrammes:howtheywork?

3!

MandatoryProgrammes:•ScienceCoreTechnologyProgramme(CTP)•BasicTechnologyResearchProgramme(TRP)•Etc….Op#onalProgrammes:•GeneralSupportTechnologyProgramme(GSTP)•Etc…(FutureLaunchersPreparatoryProgramme,MarsRobo;cExplora;on)

h]ps://indico.esa.int/indico/event/81/material/slides/16.pdf

-Generic-Applica;onspecific

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INAFHeadquarter,6-Aprile-2017! 4!

Whilsttheini#alstagesofnewtechnologydevelopment,leadinguptoexperimentalverifica#on,arepursuedthroughESA'sBasicTechnologicalResearchProgramme(TRP),theCTPexiststotakethesenewtechnologiesandapplythemtothe specific technical requirements of future science missions. CTP funded ac;vity carries them to higher stages oftechnologicalmaturity, up to full-scale engineeringmodels fully tested in relevant environmental condi;ons, ready forinclusioninthedefini;onstageofthemission–whichisthedesignphasewhichguidestheactualspacecra`construc;on.

h]p://www.esa.int/Our_Ac;vi;es/Space_Engineering_Technology/Science_Core_Technology_Programme_CTP

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Howto«request»foraTechnologicalDevelopmentAc#vity(TDAthatESAwillinsertintheTDP):oneofthepossibleop#on…

5!

As we have seen, ESA put in place the CTP to be sure that a mission will fly compliant with itsrequirements (e.g., for ATHENAbefore the adop;on due to an «early» request of TRL5wrt usualstandard)àESAhastheinterestinflyingsatellitesthatfulfilltherequirements,andinthecontextoftheCTPcanprovideresourcesforhelpingthisprocess(understandingofcri;calissues,tobesolved).It isaninterestoftheconsor;umtotransfertoESAthemessagethatcouldbepresenttechissues(i.e.,cri;cal)tobesolved:

1)  ItisfundamentaltoconvinceESAontheimportanceoftheproblemtobesolvedinthecontextofthemissionrequirements

2)  If thenecessary skillsare present in the consor;um (inside the team), it is also important toinformESAthattheconsor;umisabletosolvefortheseissues

3)  Provide to ESA from a formal point of view abrief doc having a descrip#onof the problem,expectedcosts,etc….

4)  IF1)+2)+3)areok,ESAwillemitadedicatedtender,notnecessarily«tailored»toyourscien;ficissues(inmyunderstandingtheytrytosa;sfyalsootherproductstheyalreadyhave)

CTP:scienceCoreTechnologyProgrammeHowtopar#cipate:CTPproposalsareissuedcon;nuouslythroughouttheyearonESA'sEMITSwebsite,availabletoallEuropeanfirmson a 100percent funding basis. In some cases small tomedium sized enterprises(SMEs)arefavouredassubcontractorstoprimes!OPENCOMPETITION

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EUROPEANSPACEAGENCY-SCIENCEPROGRAMMETECHNOLOGYDEVELOPMENTPLAN

PROGRAMMEOFWORKFOR2017ANDRELATEDPROCUREMENTPLANPublica;ondate:06December2016Copyright:ESAThisdocumentisprovidedforinforma;ononlyandissubjecttofutureupdates.

h`p://sci.esa.int/science-e/www/object/doc.cfm?fobjec#d=47730

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EMITS:ElectronicMailingInvita#ontoTenderSystem(sincemid1980’s).h`p://emits.sso.esa.int/emits/owa/emits.main

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TheESAEMITSwebsitehaslotofinfo….

Onceyouareinterestedinatender,youhavetodownloadthedocsbyLOGIN!INAFhasUserNameandPasswordhavinginplaceseveralcontracts.Typicallyyoudownload4docs:

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àBudget,deadlineforques;ons,deadlineforproposalsubmission(CD,hardcopynowon-linesubmission)

àHowtowritetheproposal;howitisallocatedthebudget(%ondifferentParts);ifpreliminaryworkmustbepresented;BIPR;varioustables(BiddingTeamandPriceBreakdownInforma;on,Geographicaldistribu#on,Declara;onsonCompliances,Evalua#onCriteriaandWeigh#ngFactors)

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NOPANICifyouthinkyouarenotabletocomplywiththedeadline:youcanrequest

foranewone,IFJUSTIFIED!

Poten;albiddersareencouragedtopostanexpressionof interest on EMITS (see Expression of interest) in apar;cularITT:1)tobeinformedofanydevelopmentsthattakeplace2) other companies can take these expressions ofinterest intoaccountwhenestablishing their strategyinreplyingtoanInvita#onToTender.

ForAREMBESESAhasalsoprovided«evalua#oncriteria»

Dependingonthetender,usuallyabout2,5monthsforsubmiqngtheproposalàATLEAST1monthfull#meforedi#ng,+understandingoftheproposal,seqnguptheteam,fundsnegota;oninsidetheteam,signatures…

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Thecoverle`erisabriefsummaryofthefullproposal,whereitisreportedKEYITEMof:1)  Technicalàhereyoualsostateno/partly/fullycompliancewrttheSoW2)  Management3)  Implementa;on4)  FinancialàhereyoureportforaAdvancePayment(max15%),ifany5)  Contractual6)  ConclusionàhereyoustatethatyouwanttodiscusswithESAissues,ifany,arisen7)  Eligibiltyrequirements8)  Nobenefitsrequirement9)  Biddingteamandpricebreakdowninforma;on10) Geographicaldistribu#onwithinthebiddingconsor;um11) Contactdetails,Representa;ves(TechandContractualmanagementofeachbidder)12) Keyacceptancefactorsài.e.,eachiseligible;thebidcontainsC3measure(R&D,SME)13) Declara#onofComplianceàfromthetech,managerial,financialpointofview,etc…

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ProposalselectedàNego#a#onmee#ngànowisputinwri;ngthecontractàthePMisinvitedtoregisterattheESA-P

14!

Payment in 30 daysupon received theinvoice!

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AREMBESinmoredetails…

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Ariane V (VI ?) class launcherSatellite mass ~ 5500 kg Power ~5600 W Focal length: 12 m Lifetime: 5 years (10 years)

Nandra et al. 2013 arXiv1306.2307

THEATHENAOBSERVATORY:1TELESCOPEFOR2INSTRUMENTS!

Wide Field Imager:ΔE: 125 eV Field of view: 40’ x 40’

Rau et al. 2013 arXiv1307.1709

Silicon Pore Optics:Effective area: 2m2 @ 1 keV PSF (HEW): 5’’

Willingale et al. 2013 arXiv1308.6785

X-ray Integral Field Unit: ΔE: 2.5 eV

Field of view: 5 arcmin Large array of TES cooled at 50 mK

Barret et al. 2013 arXiv:1308.6784!

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At the same time:!! Photon focusing!! High energy resolution spectra!

ATHENAX-IFU:!HighqualityX-rayop#cs!TEScamera(thousand’spixels)

As the optical CCD!

The X-ray Integral Field Unit:!the X-ray astronomy enters in a new era!!

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THEATHENAX-IFU

doi:10.1038/nature18627!

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CAD!Geant4 mass model!

photons

neut

rons

protons

electrons

Thescien;ficsignalscomefromthetop!!

Fmin =nσQAs

BiAd + BdQΩAstΔE

Thepar#clebackgroundissue:noX-raymissionhaseverflowninL2!

Credits:S.Loo(IAPS)

In this respect the main issues to be probed requestedfromtheATHENAteamtoESA:•  L2par;cleenvironment(GCR+So`protons)•  Geant4physicsvalida;on

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AREMBES: the Statement of Work.!ESA issued an ITT tender which covered “part” of the already planned ac;vi;es inside the X-IFU bkgworkpackage from the L2 environment to the GEANT4 valida;on (then the residual par;cle bkg asoutput).Fromthescien;ficpointofviewthisITTinvolvestheATHENAsatellite:X-IFU+WFI.

The Statement ofWork consists of 3 Parts, to be framed in 30Months of work (“%” relates to theallocated resources by ESA – 600 kEuro). Modulus a 10% of the overall budget for the projectmanagement,wehaveallocated:

•  Part 1 (30%, 9 Month): Analyses of radia;on effects data and experience from previous X-raymissions, consolida;onof user requirements, improvement of L2 radia;on environmentmodels, andimprovementof the relevantbasicphysicsmodels to treatpropaga;onof chargedpar;cles,photonsandradia;onbackgroundinX-raymirrorsandsurroundingspacecra`structures

•  Part2 (60%,9Month):Developmentofauser-friendly radia;onbackgroundsimulator frameworkincorpora;ngPart1outputandconsideringthespecifictechnologiesusedintheATHENAtelescopeandforeseen instruments, verifica;on of all so`ware elements, construc;on of a representa;ve ATHENAgeometrymodel,andvalida;onofthesimulatorperformance

•  Part3(10%,12Month):Thispartcoversthemaintenanceandupgradesofthedevelopedso`ware

10Ins#tu#ons/SMEsinvolved:∼599krequested!595kapprovedAc#vitykicked-offon21stMarch2016

ModelDevelopmentReview(endofPhase1)onJanuary,18,2017

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TheAREMBESconsor#um(KeyPersons).Name Institute/SME

C. Macculi INAF S. Molendi INAF S. Lotti INAF A. Argan INAF M. Laurenza INAF M. Rossi INAF D. Martella INAF T. Mineo INAF A. Bulgarelli INAF V. Fioretti INAF V. Génot IRAP F. Pajot IRAP C. Jacquey IRAP F. Lei Radmod V. Ivanchenko CERN P. Truscott Kallisto Consultancy A. Mantero SWHARD P. Dondero SWHARD B. Gianesin SWHARD S.A. Ibarmia Huete INTA P. Laurent CEA Tanja Eraerds MPE Andreas von Kienlin MPE D. Haas SRON J. Dercksen SRON J.W. den Herder SRON A. Anastasiadis NOA/IAASARS I. Georgantopoulos NOA/IAASRAS I. A. Daglis NOA/IAASARS

21!

It has been necessary to involve different skillsfrom:•  X-rayastronomers•  Geant4developers•  Plasmaphysicists•  s/wdevelopers

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Geographicdistribu#onandWBS

The colour is an institute/SME.!Due to the Tasks, our proposal involve

7 nations.!

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Organiza#onBreakdownStructure

Modulus10%oftheresourcesallocatedtotheProjectManagement,wehave:

•  Part1(30%resources,9Month)•  Part2(60%resources,9Month)•  Part3(10%resources,12Month)

Meeting Date Location Milestone Kick-off T0 ESTEC T0 PM1 End of Task 3 Italy T0 + 5M MDR: Model Development Review End of Task 4 ESTEC T0 + 9M PM2 In the course of Task 5 UK T0 + 15M PM3 End of Task 6 Spain T0 + 16M SQR: Simulator Qualification Review End of Task 7 ESTEC T0 + 18M PM4 In the course of Task 8 Telecon/WebEx T0 + 24M Final Presentation End of activity ESTEC T0 + 30M

Minimumgroupofmee;ngsrequestedbyESA

(+projectmee;ngs)

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Deliverable n.

WP

Delivery Expected date

Responsibility

Del. 0 0 Progress Reports Monthly INAF Del. 1 0 TN 1.3_a on User

Requirements to G4 T0 + 3M INAF

Del. 2 0 TN 1.3_b on User Requirements to Simulator

T0 + 9M INAF

Del. 3 0 SW-4 T0 + 30M INAF Del. 4 1.1 TN 1.1 T0 + 9M INAF Del. 5 1.2 TN 1.2 T0 + 3M Kallisto

Consultancy Del. 6 2.1 TN 2.1 T0 + 9M IRAP Del. 7 2.1 SW-1 T0 + 9M IRAP Del. 8 2.4 TN 2.2 T0 + 9M Kallisto

Consultancy Del. 9 3.1 System Requirements

Doc. T0 + 5M SWHARD srl

Del. 10 3.1 TN 3.1 T0 + 5M SWHARD srl Del. 11 4.1 SW-2 T0 + 9M SWHARD srl Del. 12 4.1 TN 4.1 T0 + 9M SWHARD srl Del. 13 5.2 DJF of Simulation

Framework T0 + 13M RadMod

Research Del. 14 5.4 TN 5.1 T0 + 16M RadMod

Research Del. 15 5.4 SW-3 T0 + 16M RadMod

Research Del. 16 5.4 SUM T0 + 16M RadMod

Research Del. 17 6.1 SVP for DJF (input to

TN 6.1) T0 + 13M INTA

Del. 18 6.2 TN 6.1 T0 + 16M Kallisto Consultancy

Del. 19 7.1 Verification rep. on its activity

T0 + 12M CEA

Del. 20 7.2 TN 7.1 T0 + 18M INAF Del. 21 7.2 TN 7.2 T0 + 18M INAF Del. 22 8.1 Updates to TN 3.1 T0 + 24M SWHARD

s.r.l. Del. 23 8.1 Updates to TN 3.1 T0 + 30M SWHARD



s.r.l. Del. 26 8.2 Updates to TN 1.1 T0 + 24M INAF Del. 27 8.2 Updates to TN 1.1 T0 + 30M INAF Del. 28 8.5 Updates to TN 3.1 T0 + 24M INAF Del. 29 8.5 Updates to TN 3.1 T0 + 30M INAF Del. 30 8.6 Updates to TN 2.1 T0 + 24M IRAP Del. 31 8.6 Updates to TN 2.1 T0 + 30M IRAP Del. 32 8.6 Updates to TN 2.2 T0 + 24M IRAP Del. 33 8.6 Updates to TN 2.2 T0 + 30M IRAP

!EachmonthaprogressreporttobesenttoESAtech.officer

Phase1closed

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Needofanupgrade?!CCN:ContractChangeNo#ce

25!

TheATHENAscienceteamrequestedtoalsoprobetheL1orbit,toprovideacomparisonbetweenL2vsL1ànewac;vitywrttheAREMBESbaselineàitneedsofaCCN.Further,duringthenego;a;onmee;ngtopicscouldbeportedinaCCN.

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h]p://space-env.esa.int/index.php/news-reader/items/AREMBES.html

•  9refereedpaper(8INAF1stauthor)•  1conferenceproceeding(1stINAF)•  4talks(2INAF)atthenextGeant4

SpaceUsers'Workshop(nextweek)In9monthsac#vity(Phase1)

TheTNwillbepapers!

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Atpresent,INAFhasseveralCTPproposal/contractinplaceforATHENAasPIorWPleader

27!

AREMBES - ATHENA Radia;on Environment Models and x-ray Background EffectsSimulators(C.Macculi,PI,IAPS)

EXACRAD - Experimental Evalua;on of ATHENA Charged Par;cle Background fromSecondaryRadia;onandSca]eringinOp;cs(S.Molendi,PI,IASF-Milano)

ASPHEA -Alignmentof SiliconPoreop;cs forHigh-EnergyAstronomy (D. Spiga, PI,OABrera)

SIMPOSiuM-Siliconporeop;csmodellingandsimula;ons(D.Spiga,PI,OABrera)

LAOF - Large area high-performance op;cal filter for X-ray instrumenta;on (M.Barbera,WPleader,UniPa/INAFPalermo)

TES Detector Development for Athena / X-IFU - Op;miza;on of a EuropeanTransi;onEdgeSensorArray(L.Piro,C.Macculi,WPleader,IAPS)

…butalsoonotherprojects:NOTexhaus#velist…CAM-Contamina;onAssessmentMicrobalance(E.Palomba,PI,IAPS)

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