ly-alpha emission line
DESCRIPTION
Ly-beta emission line. Ly-alpha emission line. LyaF Future: 3D map of LSS. SDSS-III/BOSS quasar density (20 per sq. deg.) WFMOS can do up to ~8 times denser 100 Mpc/h deep 400 times this volume in SDSS. Current: very sparse. SDSS-II quasar density (1 per sq. deg.) 100 Mpc/h deep - PowerPoint PPT PresentationTRANSCRIPT
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Ly-alpha emission lineLy-beta emission line
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LyaF Future: 3D map of LSS• SDSS-III/
BOSS quasar density (20 per sq. deg.)
• WFMOS can do up to ~8 times denser
• 100 Mpc/h deep
• 400 times this volume in SDSS
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Current: very sparse• SDSS-II
quasar density (1 per sq. deg.)
• 100 Mpc/h deep
• 400 times this volume in SDSS
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Primordial power spectrum parameters
WMAP 5-year
Eisenstein et al. BAO
Includes tensors
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Matter density-power amplitude constraint
WMAP 5-year
Eisenstein et al. BAO
Includes tensors
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Primordial power spectrum parameters
WMAP 5-year
Eisenstein et al. BAO
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Current parameter highlights (all including tensors, kp=0.05 1/Mpc,
WMAP5+Eisenstein BAO+LyaF)
(for T/S, BAO & LyaF independently find this level)
• With WMAP3, sum m_nu < 0.2 eV
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Observed (3D) power
Ideal 3D power (perfectly sampled)
Sampling noisen=surface density of lines of sight(analogous to galaxy shot noise)
Resolution
Detector noise
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Simulated 3D flux power, relative to real-space linear theory (McDonald 2003)
Bottom to top on left:
mu=
0-0.25,
0.25-0.5,
0.5-0.75,
0.75-1.0
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Theory/fitting formula for redshift-space power
• Linear theory on large scales
• Non-linearity + pressure + fingers-of-god
• Baryon wiggles simply modify P_L(k)
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Parameter dependence of 3D flux power (McDonald 2003)
Black - increased amplitude
Red - increased slope
Solid - LOS
Dotted - transverse
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Parameter dependence of 3D flux power (McDonald 2003)
Black - increased temperature
Red - increased dependence of temperature on density (gamma-1)
Solid - LOS
Dotted - transverse
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Parameter dependence of 3D flux power (McDonald 2003)
Black - increased <F>
Red - never mind (related to Jeans filtering)
Solid - LOS
Dotted - transverse
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Future BAO: Measure 3D power• Band power
measurement from BOSS
• Black: radial• Green:
transverse• Red: diagonal• Dotted: Seo &
Eisenstein non-linear smearing
• Normalizations compressed.
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Constraints vs.
resolution
R=62.5, 125, 250,2000
(This was for a WFMOS-like survey, less area than BOSS)
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Expected BAO distance scale constraints from BOSS