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Time variation w' is a critical clue to fundamental physics. Deep surveys of galaxies and SN to z 1. Large ... Corasaniti & Copeland 2002. w(a) = w0 wa(1-a) ...
subdominant candidates variety is common in Nature. may be easier to detect ... thermal (ma 10-3 eV, subdominant) otherwise: smaller ma possible [Tegmark, ...
and Gamma function (over all brightness) Zoom: 2X digital zoom ... on only when the camera in. a low light or dark environment. Infrared (IR) cameras ...
Rays originate from the object point, O, and pass through the image point, I ... The overall magnification is the product of the magnification of the separate lenses ...
Surveys monitor millions of stars for years to find rare lensing events ... 40 binary events, parallax, extended source, lensing of variable stars, etc. ...
Sound Waves ... Sound speed plummets. Wave stalls at a radius of 150 Mpc. ... A crest launches a planar sound wave, which at recombination may or may not be in phase ...
Dark matter cusps in galaxy centers, in particular absent in ... dynamical friction and smooth any cusp. in dwarf galaxies. The material is more dissipative, ...
Naively, dark energy is a late universe effect, while the CMB primarily probes ... one induced at low redshifts by a late time transition in the total equation ...
Exploding stars supernovae are bright beacons that allow us to measure ... Structure Micro-Lensing The ISM The Solar System Supernovae Star Formation ...
10 mm thick. Fused silica substrates. Data on griz filters available ... Original g-band filter in black. 25. Huan Lin Jun 13, 2008 DES Calibration Workshop ...
in quasar spectrum at z=3.7. Neutral H simulation (R. Cen) Chasing Sound Across Redshift ... 160,000 quasars. 20% of fibers. 1.5% measurement of distance to z=2.3. ...
Evolving old stellar pop. SED. Redshifted and convolved with filter ... Weak lensing at 28 gals/sq-arcmin. Two tilings/year/bandpass. In year 1-2, 100 sec/exp ...
Reach characteristic magnitude in O(100) seconds. 10. 9/5/09. DES Fermilab Director's Review ... The magnitudes may be calculated by convolving a spectrum with good ...
Methods to investigate dark energy and dark matter: SN, CMB, ... Galaxy and quasar survey. 400,000 galaxies with redshifts. Sloan Digital Sky Survey (SDSS) ...
X-ray or gamma-ray. Camera Obscura, Gemma Frisius, 1558. 1544. A Brief History of Images ... blur circle is less than the resolution of the imaging sensor. ...
... that will use a new mosaic CCD camera with 520 megapixels covering a 3 sq. deg. ... field of view on the Blanco 4m telescope at the Cerro Tololo Inter ...
2) Constraints on the mean matter density Om, the amplitude of matter ... Based on sims assume bias -25( 5)% and scatter 15( 3)% due to bulk motions. ...
with OLIVER HAHN, Marcella Carollo, Avishai Dekel. QSO clustering. DM Haloes in the Cosmic Web ... 12,000 spectra of galaxies at 1.2 z 3 with BAB 25 and chosen ...
Lopez-Cruz, Barkhouse, & Yee 2004. early-type E/S0 galaxies evolve. passively and pile-up on the ... 2D sky distribution of galaxies from the mock catalog. ...
Michael Blanton, David Hogg, Bob Nichol, Roman Scoccimarro, Ryan Scranton, ... 4000-5000 fibers, using Echidna technology, feeding multiple bench spectrographs. ...