Development of a Stron/um Iodide Coded Aperture Instrument

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NRL Development of a Stron/um Iodide Coded Aperture Instrument by Lee Mitchell, Eric Grove, Bernard Phlips Presented at NASA Future Gamma-ray Mission Workshop 3/2016

Transcript of Development of a Stron/um Iodide Coded Aperture Instrument

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DevelopmentofaStron/umIodideCodedApertureInstrument

byLeeMitchell,EricGrove,BernardPhlips

PresentedatNASAFutureGamma-rayMissionWorkshop3/2016

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Introduc/on•  DevelopmenttowardsCodedApertureSystemforshortgamma-rayburst

(sGRB)detec/onandlocaliza/on–  WideFieldofView(90deg-fullycoded)–  Imagingenergyregime20-600keV–  Detec/onupto1MeV–  ReducedSWAPtoincreasemissionopportuni/es

•  SpaceTestProgram(STP)-istheprimaryproviderofspaceflightDODspacescienceandtechnologycommunity.–  Interna/onalSpaceSta/on–  Secondarypayloads–  Dedicatedlaunchservices.

•  Stron/umIodideRadia/onInstrument(SIRI)•  ProposedDevelopmentofPrototypeStron/umIodideCodedAperture

(SICA)array•  Full-sizedInstrument(SICADA)

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Stron&umIodideRadia&onInstrument(SIRI)Detector

SBC

UnpopulatedElectronics/COMBoard

HousingSIRI1of5instruments

STPSat5

ExplodedView

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Stron&umIodideRadia&onInstrument(SIRI)

•  InstrumentDescrip/on–  SingleRMDSrI2:Eudetector(17x17x40)mm3–  SensL2x2J-seriesSiPMarray–  lowpowerCOTSMCA(Kromek)andSBC(BeagleBoneBlack)–  /mestampedeventdata

•  Objec/ves–  Studytheinternalac/va/onoftheSrI2:Euinaspaceenvironment(al/tude~500km)

–  SiPMperformanceanddegrada/onover1yrmissionlife•  CurrentSchedule

–  InstrumentassemblyandGEVStes/ng(nextfewmonths)–  Spacecradintegra/onbeginsummer2016–  Launchsummer2017,Falcon9,ESPAring

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Stron/umIodideCodedAperture

TestdetectorCrystalandSiPM

27Ucube

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SICAprototype

•  Objec/ves–  sGRBdetec/onandimaging–  intheFCFOVRate2-3/yr–  SmallinstrumentincreaseslikelihoodofSTPselec/on–  3yearsfromstarttolaunch–  Reasonableposi/onaccuracy–  Imagingregime(20–600keV)

•  Descrip/on–  DetectorPlane–8x8arrayofSrI2:Eu3.2%@662keV(pitch1.0cm)–  EachDetector-0.8cmx0.8cmx5cm–  Mask–Tantalum30x30eachelement(1cmx1cmx0.5cm)–  COTSelectronics,withsomecustommainboards–  Mask20cmfromdetectorplane–  FullyCodedFieldofView(FCFOV)=58o–  AngularResolu/on(AR)=2.9o–  Power=13W

Note:Posi/onaccuracy=AR/SNR

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Stron/umIodideCodedApertureDetectorArray(SICADA)

•  FullSizedversionof(SICA)•  Objec/ves

–  IncreasedsGRBdetec/onrate(~8/yr)overtheprototype–  Improvedposi/onalaccuracy–  Energyregime20keV–600keV–  Largerinstrumentwithbackgroundrejec/on–  SWAPandcostsstartlimitmissionop/ons

•  Descrip/on–  DetectorPlane-40x40arraypitch=1cmthickness5cm–  MaskTitanium108cmx108cmx0.5cm(pitch1cm)–  Largernumberofchannels(morecustomelectronicsrequired)–  FCFOV=90o–  AR=~2.0o(20arcminfora6sigmadetec/on)–  Mass~300kg–  Power20-30W–  Ac/veBGOshieldonbackandsidesofdetectorplane

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Stron/umIodideCodedApertureDetec/onArray(SICADA)

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SICADASimula/ons

•  Simulated1photon/cm2sGRB5ooffaxis

•  Addedinternalbackground(duetoac/va/on)

•  Needtoaddgalac/cdiffuseandalbedobackgroundcontribu/ons

Withoutinternalbackground

Withinternalbackground

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Conclusion

•  Thedura/onofsGRBs(T90<2s)associatedwithLIGOtypeeventsrequireswideFOVfordetec/on.

•  AsmallinstrumentsuchasSICAwouldallowustorapidlygetsomethingintotheSTPqueue

•  Alargermoresensi/veinstrument(SICADA)isidealbutlargerSWAPlimitsmissionopportuni/esandincreasescost