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JDEM Update

JDEM Update. Richard Griffiths (NASA HQ) JDEM Program Scientist Neil Gehrels (NASA GSFC) JDEM Project Scientist. February 3, 2010. JDEM Motivation. JDEM is a space mission to determine the nature of the dark energy that is driving the current accelerated expansion of the universe

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JDEM Update

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  1. JDEM Update Richard Griffiths (NASA HQ) JDEM Program Scientist Neil Gehrels (NASA GSFC) JDEM Project Scientist February 3, 2010

  2. JDEM Motivation • JDEM is a space mission to determine the nature of the dark energy that is driving the current accelerated expansion of the universe • Space observations provide the best opportunity for a major step forward in understanding • L2 orbit • 3-5 year mission • The time is ripe for JDEM: • Dark energy study needs large area, sensitive surveys in the NIR and visible • Space-qualified large format HgCdTe and CCD detectors are US developed technology and flight ready current acceleration

  3. JDEM Science • JDEM is an optical-IR survey mission with Dark Energy as its major goal. Ancillary science comes as a by-product of DE surveys. • JDEM must perform as a precision cosmology experiment with tight error control. DE measurements are systematics limited. • There are 3 DE major techniques. Each is best done in the stable, clear environment of space. JDEM will employ one or more of them to give 10x advance in DE. • weak lensing: large-scale imaging and photo-z survey • baryon acoustic oscillations: large-scale spectroscopy and imaging survey • supernovae: monitoring 10 deg2 field

  4. JDEM Techniques • Three most promising techniques each provide different physical observables and unique information related to DE: • Baryon Acoustic Oscillation (BAO) DA(z), H(z) direct measure (large area spectroscopic survey) • Weak Lensing (WL) DA(z), growth of structure (large area imaging & photo-z survey) • Type Ia Supernovae (SNe) DL(z) (monitoring, light curves & spectroscopy) 4

  5. JDEM NIR Surveys NIR Imaging Surveys Redshift Surveys JDEM * * JDEM JDEM provides a comprehensive data set (100's TB) to world community for ancillary science with factor 100-1000 step forward in imaging & redshift surveys 5

  6. Why Space? • The following observations that are critical to dark energy progress are impossible or infeasible to make from the ground: • Wide-field spectroscopy of the bright H-alpha line to z>1 for BAO • Supernova observations to z>1. Precision NIR light curves of all supernovae. • Wide-field survey to >25th mag in NIR for WL photo-z's • Galaxy shape measurements with small & stable PSF

  7. Two mission architectures were presented to Astro2010 in June JDEM-IDECS HgCdTe and CCD imagers, plus HgCdTe spectrometers. WL shape measurement with CCDs in visible. JDEM-Omega HgCdTe imager and spectrometers. No CCD imager. WL shape measurement with HgCdTe in space-unique NIR, at some risk. Visible photo-z data from ground. Project offices are currently studying Probe-class architectures with cost goal of $650M + launch services JDEM Configurations 7

  8. Project Activities 8 • JDEM Probe Study requested by NASA and DOE. • Wide range of payload concepts under study. Varying levels of emphasis in BAO, SNe and WL techniques • 1 - 2 of the concepts will be selected for further study • Telescope study contracts awarded to ITT and Ball Aerospace. • Determine feasible designs, perform integrated modeling and parametric cost trades, develop cost and schedule estimates.

  9. JDEM is a joint NASA-DOE mission MOU in place between NASA and DOE JDEM Project Offices have been established at GSFC and LBNL Oversight group at agency level chaired by J. Morse and D. Kovar JDEM Mission Formulation 9

  10. ISWG 10 • Interim Science Working Group (ISWG) formed in December 2009 • Members chosen from proposals submitted to NASA and DOE • Tasks include: • Advise agencies on JDEM • Assist Project in defining and assessing Probe concepts • Assist Project in choosing 1-2 Probe concepts for further development

  11. Interim Science Working Group • Co-Chairs Charles Baltay Yale U. Warren Moos Johns Hopkins U. • Members Dominic Benford GSFC Gary Bernstein U.Penn. Wendy Freedman Carnegie Obs. Chris Hirata CalTech Alex Kim LBNL Rocky Kolb U.Chicago Sangeeta Malhotra ASU Nikhil Padmanabhan Yale U. Jason Rhodes JPL Greg Tarle U.Michigan • Ex-Officio Members Neil Gehrels GSFC Michael Levi LBNL 11

  12. Current Status • JDEM's future will be determined by Astro2010 • ESA dark energy mission, Euclid, was recently recommended by ESA’s Space Science Advisory Committee to be considered by the Science Programme Committee for Phase A study (SPC meets mid-Feb). • NASA/DOE and ESA are working independently on JDEM and Euclid.

  13. JDEM Probe Master Schedule

  14. Summary • The time is right for JDEM • New technology large-format detectors are now space qualified, enabling wide-field space surveys • Space observations provide the needed clean systematics control. JDEM promises the best path forward for dark energy understanding in the coming decade. • Awaiting recommendations for dark energy science and JDEM from Astro2010. Dark energy is the mystery of our time. Solving it will lead to a new era of understanding how the universe works and what our cosmic fate is

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