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Redshift -Space Enhancement of LOS Baryon Acoustic Oscillations in the SDSS-MGS. Reporter: Haijun Tian Alex Szalay, Mark Neyrinck, Tamas Budavari. arXiv:1011.2481. Outline. Background Redshift Space in Linear Theory Measurement from simulations Measurement from SDSS
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Redshift-Space Enhancement of LOS Baryon Acoustic Oscillations in the SDSS-MGS Reporter: Haijun Tian Alex Szalay, Mark Neyrinck, Tamas Budavari arXiv:1011.2481
Outline • Background • Redshift Space in Linear Theory • Measurement from simulations • Measurement from SDSS • Quantifying the redshift space features • Conclusion
Definition • Acoustic Oscillations: the competition between the photon pressure and the baryons gravitational collapse prior to the epoch of recombination • The Redshift Space Distortion: Due to the peculiar velocity Smaller Scale: dominated by nonlinear (FoG’s) Larger Scale: present as compression effect along LOS It is relative to Real Space
Redshift Distortion From SDSS Project From 2DF Project
Detect BAO for the First time • Eisenstein et al (2005) – LRG
SDSS Redshift Samples • Main Galaxies 800K galaxies, high sampling density, but not too deep Volume ~ 0.12 Gpc3 • Luminous Red Galaxies(“Sweet Spot”) 100K galaxies, color and flux selected m_r < 19.5, 0.15 < z < 0.45, close to volume-limited Lower density , Volume > 2 Gpc3 Good balance of volume and sampling • Quasars 20K QSOs, cover huge volume, but too sparse
A Recent Controversy on Bump_LOS Kazin(2010) Gaztanaga et al(2009)
(r) from linear theory + BAO • Mixing of 0 , 2 and 4 • Along the line of sight
What can predict • Nearby the LOS, the distortions sharpen the “bumpy” feature, and much weaker, much further from the LOS. • Overall smoothly shifts towards negative along the LOS, and towards positive in the transverse.
Projection and Slicing Theorem • The basis of CAT-SCAN
Methods to estimate lower Dimensional • _3D _2D _1D (LOS) • P(k)_3D P(k)_2D _2D _1D • Slice sample(2D) _2D average _1D • Slice sample(2D)P(k)_2D average P(k) _2D _1D • Principally, all the cases will contain the same _LOS, nevertheless the covariance between the bins estimated in different ways will be somewhat different.
Measurement From Simulation • Millennium Simulation(MS) Size: 500 h-1Mpc a bit small, 2563 Grid R-mag: < -20 (absolute) Mean density: 0.02 (h-1Mpc)-3 • Particle-Mesh(PM) dark-matter Simulations Size: 1024 h-1Mpc, 100 2563 particles • 1400 Gaussian Simulations Size: 768 h-1Mpc, 16 h-1Mpc thickness(at 370 h-1Mpc)
Correlation function from MS • MS is divided into 3 x 64 slices, 8 h-1Mpc • For Redshift Space:
Correlation function from100 PMs • Real Space: 3 orientations, 8 h-1Mpc • Redshift Space: 6 orientations(3 possible LOS axes, times 2 slice orientations contain LOS)
What can we find from simulations • Linear-theory distortions in 2D sharpen the baryon bump relative to the real space. • While fingers of god(non-linear) degrade all features, even away from LOS. • Error bars for the LOS BAO bump are slightly reduced compared with the angle-averaged bump. • Even in 3D, in redshift space have a sharper BAO bump than in 2D. • Redshift-space distortions tend to amplify the bump sharpness, especially along the LOS.
Measurement from SDSS • SDSS DR7 MGS, Stripes 9 through 37, Northern cap • 0.001<z<0.18, Z_conf>0.9, Z_err<0.1 • Remove all the objects in the incomplete areas • About 527K objects. • 17M random galaxies • Spatial weighting • From 0 to 165deg, 15deg increments,12 angular orientations, 2.5deg thickness, 20deg<width<80deg, 660slices
Computing and Correlations • Estimator: • Done on an GPU(NVIDIA’s CUDA) 400 trillions galaxy/random pairs • Brute force massively parallel code much (hundreds of times) faster than tree-code • All done inside the JHU SDSS database • Based on the Buffon’s needle(Buffon 1777), figure out the number slices on average that enter the LOS.
Contour of Average (,) of the 660 2.5deg slices of SDSS galaxies(left),and the full 3D (right) 100Mpc/h<dist<750Mpc/h 300 Mpc/h <dist<750 Mpc/h
Angle-average and LOS 1D for low-resolution PM, MS, SDSS sample, angle-average(top), and LOS(6deg)
The Bump at160Mpc/h 300 Mpc/h <dist<750 Mpc/h 50<dist<300 Mpc/h
S/N of wavelet transform The S/N of the wavelet transform . S/N, 1400 Gaussian simulations, box_size:768Mpc/h, cell_size:2Mpc/h. The S/N for the SDSS real sample
[top left] The linear theory redshift space (,), [top right] The mean PM redshift space (,), [middle] The mean MS redshift space (,), [bottom] The mean SDSS redshift space (,),
S/N Frequency 1400 Gaussian simulations, SDSS-like Volume, ~40% of the simulations: S/N 2.2-sigma, LOS ~ 70% , S/N 4-sigma, flat weighting.
12 orientations DOF: 12/9.3 = 1.3(LOS) 12/1.7 = 7 (flat) S/N: 9.0 +/- 7.9 (LOS) 5.2 +/- 2. (flat)
Strong Non-Linear Infall (55Mpc) Distribution of 1D wavelet coefficients over the 660 slices, Mexican Hat • Centered at 55 h-1Mpc, 25 h-1Mpc wide,
Far Side Infall (140Mpc/h) • Centered on 140 h-1Mpc, width 25 h-1Mpc • Still shows some skewness
Conclusion • Redshift space distortions amplify and sharpen features along the line of sight • 4 detection of BAO in SDSS DR7 MGSat around 110 h-1Mpc, potentially constraining the equation of state at low z • Trough at 55 h-1Mpc indicates effects of nonlinear infall on these scales
Cosmology used M = 0.279 L = 0.721 K = 0.0 h= 0.701 w0 = -1