Testing the Standard Model of Cosmology Using BAO data - KIAS

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Model Independent Reconstruction of H(z) Smoothing Supernovae data Real time cosmology Age of passively evolving galaxies Volume distance from baryon acoustic oscillation measurements
Deriving h(z) from BAO Observable Effective dilation distance Comoving sound horizon at baryon drag epoch
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: Model Independent Reconstruction of
Page 27 and 28: Deriving h(z) from BAO
Page 29 and 30: Deriving h(z) from BAO Om diagnosti
Page 31 and 32: Alcock-Paczynski Measurement • An
Page 33 and 34: Combining the information from supe
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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