WFIRST- AFTA: European Interests
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1 WFIRST- AFTA: European Interests Mark Cropper Mullard Space Science Laboratory University College London
2 Contents 1. WFI interests Europe- wide 2. Coronagraph interests, UK only see Anthony BoccaleJ s talk also 2
3 Europe and WFI: who Following groups were canvassed, mostly based on JWST NIRSpec and Euclid Germany: Bender (MPE), Rix (MPIA) Spain: Castander (Barcelona) France: le Fevre (LAM), Mellier (IAP) Italy: CimaJ (Bologna), Scaramella (Rome) UK: Sharples (Durham), Wright (UKATC), Davies (Oxford), Nichol (Portsmouth), Cropper (MSSL- UCL) All approached were asked if there were any others they knew who might be interested 3
4 Europe and WFI: who Following groups were canvassed, mostly based on JWST NIRSpec and Euclid Germany: Bender (MPE), Rix (MPIA) Spain: Castander (Barcelona) France: le Fevre (LAM), Mellier (IAP) Italy: CimaJ (Bologna), Scaramella (Rome) UK: Sharples (CfAI- Durham), Wright (UKATC), Davies (Oxford), Nichol (Portsmouth), Cropper (MSSL- UCL) All approached were asked if there were any others they knew who might be interested Those in blue replied with an expression of interest 4
5 IFU: Durham interest, NIRSpec Heritage IFU engineering model structure IFU opmcs mounted inside cryo- test facility for the NIRSpec IFU CollaboraMon with SSTL Durham CfAI lead in: conceptual design opmcs manufacture thermal vac test (35K) 30 slices 3.0 x 0.1 WFE < 100nm Ra < 5-10nm For WFIRST: high TRL low risk WFIRST- AFTA SDT MeeMng #5 20 November
6 Durham Centre for Advanced InstrumentaMon CapabiliMes: Opto- mechanical Design 5- axis diamond machining & metrology Thermal- vac tesmng 5- axis diamond diamond machining facility Specific interests: Integral field unit(s) gold coated opmcs for 8 of the 24 VLT- KMOS IFU channels 6
7 Laboratoire d Astrophysique de Marseille: interests in WFIRST- WFI Technical interests WFI design, manufacturing, tests IFU spectrograph: slicer, disperser, mechanical structure Opto- mechanical systems: opmcs, structure, Science & ground segment interests ExperMse in deep spectroscopy survey for cosmology and galaxy evolumon IFU spectroscopy processing MulM- wavelength analysis: photometric redshifs, SED fijng, Spectra analysis: redshifs, velocity maps, ExperMse on relevant space hardware: Herschel SPIRE FTS Lead ins)tute Euclid- NISP infrastructure for integramon and tests in space environment New 90m 3 vacuum chamber (all tests for Euclid- NISP) Euclid- NISP 90m 3 Space tes<ng chamber 7
8 IFU spectrograph prototype developed for SNAP study with CPPM and LBNL Prototype developed and tested at LAM Funded by CNES, CNRS, LBNL Main space requirements (cold, vibramon) samsfied TRL~6 as evaluated by CNES- chaired panel, including high surface accuracy glass slicer λ=900nm item specifica)on FOV Pixel size Spect Res 4 x ~ x,y SimulaMon λ x,y demonstrator λ Wavelength µm OperaMng Temperature 140 K +/-? Camera F/D F/36 8
9 CalibraMon Unit: MSSL interest, NIRSpec Heritage highly specified opmcal and bandpass- controlled performance in 1 5µm band low- dissipamon light sources comb and broadband filters delivered under contract to Astrium Germany NIRSpec CalibraMon Unit Flight Model 9
10 Mullard Space Science Lab, University College London NIRSpec ground calibramon cryo- GSE Over 50 satellite missions with NASA, ESA, JAXA, USSR/ Russia, China, India Recent relevant (cryogenic) missions: ISO LWS Herschel SPIRE JWST NIRSpec Gaia Swif UVOT Euclid (VIS instrument lead) Last NASA- led missions (JWST) Cassini CAPS SwiD UVOT GOES- SXI, - N, - O, - P Cryogenic mk ADR cryocoolers Science: astrophysics and cosmology 10
11 Spanish interests in WFIRST- WFI A consormum of Spanish insmtumons in Barcelona (ICE, IFAE) and Madrid (CIEMAT, IFT) are interested in a possible parmcipamon in WFIRST This consormum is focused on Dark Energy related research It is currently involved in several Dark Energy experiments: DES, PAU, DESI and Euclid The consormum acmvely parmcipates on several aspects of these projects like management, planning, instrumental development and construcmon, sofware development and scienmfic coordinamon and exploitamon We are interested in possible parmcipamon in the WFIRST WFI in the areas of mechanics, electronics and/or control sofware Euclid: leading FWA (Filter Wheel Assembly) of NISP and SimulaMons OrganizaMon Unit in Science Ground Segment; also, host the Spanish Data Centre 11
12 Spain: Dark Energy Experiments InstrumentaMon heritage DECam: front- end electronics and guider sofware PAUCam on WHT: overall design and construcmon: mechanics, electronics, sofware control also, DESI: negomamng leadership in the GFA: guiding, focus and alignment WFIRST- AFTA SDT MeeMng #5 20 November
13 InsMtute of Cosmology and GravitaMon (ICG) University of Portsmouth: interests in WFIRST Project and sofware experience Significant science leadership roles in DES, SDSS, DESI and Euclid Development of IFU data processing pipeline for SDSS MaNGA (IFU) Founding members of GalaxyZoo and conmnued development of cimzen science projects under Zooniverse Joint SN light curve analysis between DES and VISTA WFIRST interests IFU spectroscopy processing SN classificamon and analysis, leading to improved systemamcs (cosmology) and astrophysics (discoveries) Redshif determininamon from slitless spectroscopy Precision Large scale structure measurements (masks, esmmaorts, mocks) ExperMse on relevant space missions: Lead of galaxy clustering SWG in Euclid BAO scienmst on Euclid EST GalaxyZoo:Hubble 13
14 UK Science Interests: WFI UK has strong track record in cosmology; in parmcular heritage in redshif surveys (2dFGS, SDSS) in the weak lensing probe in Euclid (Science Working Group leads, Science Ground Segment, VIS instrument lead) in the galaxy clustering probe in Euclid (SWG lead) hence is highly interested in scienmfic complementarity offered by WFIRST- AFTA Supernova science is not supported by Euclid significant interest from UK Supernova community who have leading roles in key on- going SN surveys e.g. Portsmouth is leading the DES search and there is strong involvement in the PanSTARRS transient survey (Belfast, Southampton, Oxford). ExperMse in SN cosmology and SN astrophysics Not forgejng extensive UK galaxy evolumon interests In pracmce: involvement in WFIRST- AFTA science working groups would be welcomed Science links to ground segment sofware development 14
15 UK Interests in Coronagraph UK technology interest centred on e2v detector capability allied with research capability at Open Univ CEI MSSL- UCL camera capability (Eddington, Gaia, Euclid, PLATO) Highly integrated approach to system design, high performance, radiamon mimgamon Experience with operamon of and space qualificamon of L3CCDs via Gaia RVS programme (MSSL- UCL and CEI- OU partnership) Current WFIRST contract with CEI- OU on L3CCD development Euclid 12- channel camera electronics Science interests based on PLATO involvement at MSSL- UCL, Warwick, Cambridge, Open University 100 L3CCD97 provided by e2v for Gaia- RVS detector qualificamon 15
16 Summary Significant interest in WFI across Europe in both instrumentamon and science strong Euclid complementarity track record parmcularly with JWST instruments involvement in science working groups UK interests in Coronagraph science complementarity to PLATO track record in CCDs and large space CCD cameras 16
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