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Cross-correlations of the Lyα Forest with Weak-lensing Convergence. Analytical Estimates of Signal-to-noise Ratio and Implications for Neutrino Mass and Dark Energy

  • Authors: Alberto Vallinotto, Matteo Viel, Sudeep Das, and David N. Spergel

Vallinotto et al. 2011 The Astrophysical Journal 735 38.

  • Provider: AAS Journals

Caption: Figure 1.

Absolute value of the correlator along a single line of sight as a function of the source redshift z and of the length of the measured spectrum Δ z, for convergence maps reconstructed from Planck (left panel, k C = 0.021   h Mpc −1) and ACTPOL (right panel, k C = 0.064   h Mpc −1). The value of the resolution of the QSO spectrum is the one predicted for SDSS-III, k L = 1.9  h Mpc −1. Also, we set k l = 0.01  h Mpc −1. To make the physics of structure formation apparent, we turn off the IGM physics by setting A = β = 1 (it is straightforward to rescale the values of the correlator to reflect different values of A and β).

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