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Observational Cosmology at Fermilab: Sloan Digital Sky Survey Dark Energy Survey SNAP

Observational Cosmology at Fermilab: Sloan Digital Sky Survey Dark Energy Survey SNAP. Gajus Miknaitis EAG, Fermilab. Sloan Digital Sky Survey (SDSS). Motivation : study the distribution of matter in the universe by measuring the distribution of galaxies in space (2D + redshift).

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Observational Cosmology at Fermilab: Sloan Digital Sky Survey Dark Energy Survey SNAP

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  1. G. Miknaitis SC2006, Tampa, FL Observational Cosmology at Fermilab: Sloan Digital Sky Survey Dark Energy Survey SNAP Gajus Miknaitis EAG, Fermilab

  2. G. Miknaitis SC2006, Tampa, FL Sloan Digital Sky Survey (SDSS) Motivation: study the distribution of matter in the universe by measuring the distribution of galaxies in space (2D + redshift) 125 Mpixel Imaging Cameraa Spectrograph fed by 640 optical fibers SDSS 2.5 m Telescope at Apache Point Observatory

  3. G. Miknaitis SC2006, Tampa, FL Sloan Digital Sky Survey (SDSS) Motivation: study the distribution of matter in the universe by measuring the distribution of galaxies in space (2D + redshift) CfA Redshift Survey (1986) Imaging camera: find galaxies, measure their angular positions

  4. G. Miknaitis SC2006, Tampa, FL Sloan Digital Sky Survey (SDSS) Motivation: study the distribution of matter in the universe by measuring the distribution of galaxies in space (2D + redshift) CfA Redshift Survey (1986) Multi-object spectrograph: measure galaxy redshifts distance ≈ redshift Imaging camera: find galaxies, measure their angular positions

  5. After ~5 years of operation, SDSS has: imaged more than 8,000 square degrees of the sky in five bandpasses detected nearly 200 million celestial objects measured spectra of more than 675,000 galaxies, 90,000 quasars, and 185,000 stars SDSS data set G. Miknaitis SC2006, Tampa, FL

  6. data: Sloan Digital Sky Survey and the Bright Star Catalog visualization: David W. Hogg (NYU) with help from Blanton, Finkbeiner, Padmanabhan, Schlegel, Wherry

  7. G. Miknaitis SC2006, Tampa, FL SDSS & Large Scale Structure power spectrum of matter 1 megaparsec

  8. G. Miknaitis SC2006, Tampa, FL Scientific impact of the SDSS • As of May 30, 2006, 1080 refereed, published papers use the Sloan Digital Sky Survey data. ½ of these papers are authored by people not in the collaboration, with public SDSS data access from our servers. • Over 31,000 citations of these papers in the literature. • 22 SDSS papers with more than 200 citations • Some science highlights • State-of-the-art Large Scale Structure measurements • 3D power spectrum; baryonic acoustic oscillations • Catalog of 105quasars out to z≈7 • Reionization of the universe at z=7 (Gunn-Peterson effect) • Catalog of 106galaxy clusters to z=0.5 • Tidal tails and stellar streams in our galaxy • Discovery of many rare low-mass dwarf stars

  9. G. Miknaitis SC2006, Tampa, FL This is the brightest known image of a galaxy from the early Universe. Furious star formation makes the galaxy luminous, but the image is bright because the gravty of the foreground galaxy (red) acts as a natural telescope, focusing its light. The newly discovered galaxy, seen as an arc of four elongated images that encircle the foreground lens, offers a rare window into the state of the Uniferse two billion years after the big bang.

  10. SDSS I: april 2000 - june 2005 completed SDSS II: july 2005 - july 2008 SDSS II: The Sequel G. Miknaitis SC2006, Tampa, FL

  11. G. Miknaitis SC2006, Tampa, FL SDSS II: components • SDSS “legacy”: complete the original imaging and spectroscopy survey • SEGUE: study the (dark matter) halo of the Milky Way • Supernovae: survey to discover ~200 SNe to probe the expansion history of the universe (dark energy)

  12. G. Miknaitis SC2006, Tampa, FL 3. Supernovae & Dark Energy • Type Ia supernovae are standard(izable) candles. • By measuring their brightness and cosmological redshift, we can trace the expansion rate & thus infer the make-up of the universe as a function of time. • Initial SN experiments found surprisingly that the universe appears to be speeding up, fueled by gravitationally repulsive “dark energy”.

  13. G. Miknaitis SC2006, Tampa, FL 3. SDSS II Supernovae • SDSS well-suited to finding SNe at moderate redshifts that are difficult for other experiments • Build up large (~200) sample of well-observed supernovae to study dark energy and better understand the supernova population • Study systematics which are increasingly important with larger samples Astier '06

  14. G. Miknaitis SC2006, Tampa, FL Finding and measuring supernovae supernova 1. Take an image 2. Take another image later 3. Subtract the two 3. 2. 1. subtraction artifact

  15. G. Miknaitis SC2006, Tampa, FL Finding and measuring supernovae supernova 1. Take an image 2. Take another image later 3. Subtract the two 4. Continue taking images to measure supernova “light curve” 3. 2. 1. 4. subtraction artifact

  16. G. Miknaitis SC2006, Tampa, FL SDSS II first year supernova yield: 139 spectroscopically confirmed Type Ia Supernovae from the Fall 2005 Season Analysis is underway 2 more years to go!

  17. Fermilab is engaged in a variety of exciting observational astrophysics and cosmology projects SDSS is the world leader in studies of large scale structure of the universe (and many other fields of astronomy) SDSS-II will enhance our understanding of two of the today's greatest mysteries in cosmology: Dark Matter and Dark Energy In the future, Dark Energy Survey and Supernova Accleration Probe will provide precise constraints on the nature of Dark Energy Summary G. Miknaitis SC2006, Tampa, FL

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