Cosmic Surveys – Rich Kron - Fermilab Center for Particle ...

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S. Allam HST Cy16Sup GO-11974 Fermilab science: Luminous Red Galaxies clusters supernovae lensing photometric redshifts structure of the Milky Way Fermilab technical: calibration simulations pipelined data processing data quality assurance accessible databases project management
SDSS-III: baryon acoustic oscillations discovered in SDSS spectroscopic data: error in length scale from 2005 data ~ 4% at z = 0.35. Can get 7x SDSS volume with a new survey with upgraded hardware (smaller fibers, more fibers, and extended red sensitivity). 1.5 x 10 6 galaxies, 1% error on length scale at z = 0.6. Also look for BAO in Lyman α forest using a denser network of quasars enabled by better blue CCD’s. 160,000 quasars, 1.5% error on length scale at z = 2.2.
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Page 4 and 5: This high impact is due to several
Page 6 and 7: SEGUE (Sloan Extension for Galactic
Page 10 and 11: “hyper-velocity star” Brown, W.
Page 12 and 13: SNe Survey N S Use the SDSS 2.5m te
Page 14 and 15: Hubble Diagram with SDSS SNe 103 SN
Page 18: Bright time can be well used with a
Page 21 and 22: • Study Dark Energy using The Dar
Page 23 and 24: Zekser, K. et al. 2006 ApJ 640, 639
Page 26 and 27: Fermilab is the host institution fo
Page 28 and 29: Fermilab UIUC/NCSA The University o
Page 30 and 31: Study Groups: Theory/Combined Metho
Page 32 and 33: SDSS and DES imaging comparison pix

Cosmic Surveys – Rich Kron - Fermilab Center for Particle ...

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