All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
| Autor: | Xavier, H. S., Costa-Duarte, M. V., Balaguera-Antolínez, A., Bilicki, M. |
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| Rok vydání: | 2018 |
| Předmět: | |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1088/1475-7516/2019/08/037 |
| Popis: | Aiming to extract cosmological information from linear scales of the WISE$\times$SuperCOSMOS photometric redshift catalog, we perform a characterization of the systematic effects associated with stellar content, evidencing the presence of contamination and obscuration. We create an integrated model for these effects (which together we call `usurper contamination'), devise a method to remove both of them simultaneously and show its functionality by applying it to a set of mock catalogs. When administered to WISE$\times$SuperCOSMOS data, our method shows to improve the measurements of angular power spectra on scales $\ell\lesssim15$ and the extraction of cosmological parameters therefrom, even though a significant excess of power remains at these scales. When ignoring scales $\ell<15$, we still find strong indications of systematics, albeit these can be localized in the southern equatorial hemisphere. An independent analysis of the northern hemisphere at $\ell\geq 15$ agrees with a $\Lambda$CDM model with parameters from the Planck satellite and gives $\Omega_{\mathrm{c}}=0.254\pm0.020$ and $\Omega_{\mathrm{b}}<0.065$ at 95% confidence limit when combined with priors on $H_0$, $A_s$ and $n_s$. Comment: 33 pages, 20 figures, 5 tables. Accepted for publication in JCAP |
| Databáze: | arXiv |
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