scholarly journals Using multipoles of the correlation function to measure H(z), DA(z) and  (z) from Sloan Digital Sky Survey luminous red galaxies

2013 ◽  
Vol 431 (3) ◽  
pp. 2634-2644 ◽  
Author(s):  
C.-H. Chuang ◽  
Y. Wang
2007 ◽  
Vol 378 (3) ◽  
pp. 1196-1206 ◽  
Author(s):  
Gauri V. Kulkarni ◽  
Robert C. Nichol ◽  
Ravi K. Sheth ◽  
Hee-Jong Seo ◽  
Daniel J. Eisenstein ◽  
...  

2012 ◽  
Vol 8 (S295) ◽  
pp. 185-185
Author(s):  
A. Ratsimbazafy ◽  
C. Cress ◽  
S. Crawford ◽  

AbstractLuminous Red Galaxies (LRGs) have old, red stellar populations often interpreted as evidence of a formation scenario in which these galaxies form in a single intense burst of star formation at high redshift. By measuring the average age of LRGs at two different redshifts, one can potentially measure the redshift interval corresponding to a time interval and thus measure the Hubble parameter H(z) ≈ −(1 + z)−1 Δ z/Δt (as in Jimenez & Loeb). The goal of this project is to measure directly the expansion rate of the universe at the redshift range 0.1 < z < 1.0 within 3% precision. We explore the age-dating of Sloan Digital Sky Survey LRGs using the stellar population models of Lick absorption line indices after stacking spectra in redshift bins to increase the signal-to-noise. We also use the method of full spectral fitting to measure the ages of LRGs observed with the Southern Africa Large Telescope (SALT).


2011 ◽  
Vol 417 (4) ◽  
pp. 3103-3104 ◽  
Author(s):  
◽  
Beth A. Reid ◽  
Will J. Percival ◽  
Daniel J. Eisenstein ◽  
Licia Verde ◽  
...  

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