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

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This high impact is due to several factors: freely accessible database (dr7: arXiv 0812.0649) processing and calibrations: science-ready data uniform and high-quality data large footprint on the sky overlap with other major surveys (2MASS, GALEX) data useful across many fields of astronomy ----------way the telescope is used SDSS Collaboration as a scientific team
SDSS-II (2005 - 2008) extension survey: same instrumentation, same target-selection for Legacy, improvements to processing software for Legacy. Legacy required 1/3 of the total time to “fill the gap.” The other 1/3 and 1/3 were for:
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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 16 and 17: S. Allam HST Cy16Sup GO-11974 Fermi
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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