1. The one-dimensional Lyα forest power spectrum from BOSS
- Author
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Palanque-Delabrouille, N, Yèche, C, Borde, A, Le Goff, JM, Rossi, G, Viel, M, Aubourg, E, Bailey, S, Bautista, J, Blomqvist, M, Bolton, A, Bolton, JS, Busca, NG, Carithers, B, Croft, RAC, Dawson, KS, Delubac, T, Font-Ribera, A, Ho, S, Kirkby, D, Lee, KG, Margala, D, Miralda-Escudé, J, Muna, D, Myers, AD, Noterdaeme, P, Pâris, I, Petitjean, P, Pieri, MM, Rich, J, Rollinde, E, Ross, NP, Schlegel, DJ, Schneider, DP, Slosar, A, and Weinberg, DH
- Subjects
cosmology: observations ,large-scale structure of Universe ,intergalactic medium ,cosmological parameters ,astro-ph.CO ,Astronomy & Astrophysics ,Astronomical and Space Sciences - Abstract
We have developed two independent methods for measuring the one-dimensional power spectrum of the transmitted flux in the Lyman-α forest. The first method is based on a Fourier transform and the second on a maximum-likelihood estimator. The two methods are independent and have different systematic uncertainties. Determination of the noise level in the data spectra was subject to a new treatment, because of its significant impact on the derived power spectrum. We applied the two methods to 13 821 quasar spectra from SDSS-III/BOSS DR9 selected from a larger sample of over 60 000 spectra on the basis of their high quality, high signal-to-noise ratio (S/N), and good spectral resolution. The power spectra measured using either approach are in good agreement over all twelve redshift bins from 〈z〉 = 2.2 to 〈z〉 = 4.4, and scales from 0.001 km s-1 to 0.02 km s-1. We determined the methodological andinstrumental systematic uncertainties of our measurements. We provide a preliminary cosmological interpretation of our measurements using available hydrodynamical simulations. The improvement in precision over previously published results from SDSS is a factor 2-3 for constraints on relevant cosmological parameters. For a ΛCDM model and using a constraint on H0 that encompasses measurements based on the local distance ladder and on CMB anisotropies, we infer σ8 = 0.83 ± 0.03 and ns = 0.97 ± 0.02 based on Hi absorption in the range 2.1 < z < 3.7. © ESO, 2013.
- Published
- 2013