Testing the Standard Model of Cosmology Using BAO data - KIAS

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C. Blake et. al, in prepration, WiggleZ Survey: Alcock-Paczynski measurement Amplitude of systematic errors in measurements of the scale distortion parameter F(z) in four redshift slices relative to its fiducial value F_fid (FLCDM with matter density of 0.27), marginalized over the growth rate and galaxy bias b^2.
Combining the information from supernovae data and AP measurements Smoothing method reconstruct D_A(z) using supernovae data in a model independent way. (Shafieloo et al 2006, Shafieloo 2007, Shafieloo and Clarkson 2010) Assumption of curvature (here assuming flat universe) allow us to relate h(z) and distance measurements. AP measurements of distortion parameter F(z) put additional constraints on the reconstructed results through consistency check between the D_A(z) and H(z). Smoothing method can be modified to include SN Ia and AP measurements simultaneously to reconstruct the expansion history of the universe.
Page 1 and 2: Testing the Standard Model of Cosmo
Page 3 and 4: Standard Model of Cosmology Vanilla
Page 5 and 6: Beyond the Standard Model of Cosmol
Page 7 and 8: Parameter estimation within a cosmo
Page 9 and 10: Dark Energy Reconstruction • Any
Page 11 and 12: Late Universe and Dark Energy Model
Page 13 and 14: Y. Gong, JCAP (2005)
Page 15 and 16: wz () =−0.7 wz ( ) =−1.3 2 2 3
Page 17 and 18: To find cosmological quantities and
Page 19 and 20: Method of Smoothing A. Shafieloo, U
Page 21 and 22: h(z) Uncorrelated estimation of the
Page 23 and 24: Model Independent Reconstruction of
Page 25 and 26: Deriving h(z) from BAO Observable E
Page 27 and 28: Deriving h(z) from BAO
Page 29 and 30: Deriving h(z) from BAO Om diagnosti
Page 31: Alcock-Paczynski Measurement • An
Page 35 and 36: (Present)t Standard Model of Cosmol
Page 37 and 38: Conclusion • BAO links the early

Testing the Standard Model of Cosmology Using BAO data - KIAS

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