Volume 614, June 2018
|Number of page(s)||11|
|Section||Cosmology (including clusters of galaxies)|
|Published online||08 June 2018|
The impact of Lyman-α radiative transfer on large-scale clustering in the Illustris simulation
Scuola Normale Superiore,
Piazza dei Cavalieri 7,
2 Institut fuer Astrophysik, Georg-August Universität Goettingen, Friedrich-Hund-Platz 1, 37075 Goettingen, Germany
3 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Starße 1, 85740 Garching bei München, Germany
Accepted: 5 February 2018
Context. Lyman-α emitters (LAEs) are a promising probe of the large-scale structure at high redshift, z ≳ 2. In particular, the Hobby-Eberly Telescope Dark Energy Experiment aims at observing LAEs at 1.9 < z < 3.5 to measure the baryon acoustic oscillation (BAO) scale and the redshift-space distortion (RSD). However, it has been pointed out that the complicated radiative transfer (RT) of the resonant Lyman-α emission line generates an anisotropic selection bias in the LAE clustering on large scales, s ≳ 10 Mpc. This effect could potentially induce a systematic error in the BAO and RSD measurements. Also, there exists a recent claim to have observational evidence of the effect in the Lyman-α intensity map, albeit statistically insignificant.
Aims. We aim at quantifying the impact of the Lyman-α RT on the large-scale galaxy clustering in detail. For this purpose, we study the correlations between the large-scale environment and the ratio of an apparent Lyman-α luminosity to an intrinsic one, which we call the “observed fraction”, at 2 < z < 6.
Methods. We apply our Lyman-α RT code by post-processing the full Illustris simulations. We simply assume that the intrinsic luminosity of the Lyman-α emission is proportional to the star formation rate of galaxies in Illustris, yielding a sufficiently large sample of LAEs to measure the anisotropic selection bias.
Results. We find little correlation between large-scale environment and the observed fraction induced by the RT, and hence a smaller anisotropic selection bias than has previously been claimed. We argue that the anisotropy was overestimated in previous work due to insufficient spatial resolution; it is important to keep the resolution such that it resolves the high-density region down to the scale of the interstellar medium, that is, ~1 physical kpc. We also find that the correlation can be further enhanced by assumptions in modeling intrinsic Lyman-α emission.
Key words: radiative transfer / galaxies: high-redshift / large-scale structure of Universe
© ESO 2018
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