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               <dc:title>Constraints on primordial non-Gaussianity from large scale structure probes</dc:title>
               <dc:creator>Xia, Jun-Qing</dc:creator>
               <dc:creator>Baccigalupi, Carlo</dc:creator>
               <dc:creator>Matarrese, Sabino</dc:creator>
               <dc:creator>Verde, Licia</dc:creator>
               <dc:creator>Viel, Matteo</dc:creator>
               <dc:subject>Cosmologia</dc:subject>
               <dc:subject>Astrofísica</dc:subject>
               <dc:subject>Cosmology</dc:subject>
               <dc:subject>Astrophysics</dc:subject>
               <dc:description>In this paper we measure the angular power spectra Cℓ of three high-redshift large-scale structure probes: the radio sources from the NRAO VLA Sky Survey (NVSS), the quasar catalogue of Sloan Digital Sky Survey Release Six (SDSS DR6 QSOs) and the MegaZ-LRG (DR7), the final SDSS II Luminous Red Galaxy (LRG) photometric redshift survey. We perform a global analysis of the constraints on the amplitude of primordial non-Gaussianity from these angular power spectra, as well as from their cross-correlation power spectra with the cosmic microwave background (CMB) temperature map. In particular, we include non-Gaussianity of the type arising from single-field slow roll, multifields, curvaton (local type), and those which effects on the halo clustering can be described by the equilateral template (related to higher-order derivative type non-Gaussianity) and by the enfolded template (related to modified initial state or higher-derivative interactions). When combining all data sets, we obtain limits of fNL = 48±20, fNL = 50±265 and fNL = 183±95 at 68% confidence level for local, equilateral and enfolded templates, respectively. Furthermore, we explore the constraint on the cubic correction gNLphgr3 on the bias of dark matter haloes and obtain a limit of −1.2 × 105 &lt; gNL &lt; 11.3 × 105 at 95% confidence level.</dc:description>
               <dc:date>2019-01-23T10:48:36Z</dc:date>
               <dc:date>2019-01-23T10:48:36Z</dc:date>
               <dc:date>2011</dc:date>
               <dc:date>2019-01-23T10:48:36Z</dc:date>
               <dc:type>info:eu-repo/semantics/article</dc:type>
               <dc:type>info:eu-repo/semantics/acceptedVersion</dc:type>
               <dc:relation>Versió postprint del document publicat a: https://doi.org/10.1088/1475-7516/2011/08/033</dc:relation>
               <dc:relation>Journal of Cosmology and Astroparticle Physics, 2011, vol. 08, p. 033</dc:relation>
               <dc:relation>https://doi.org/10.1088/1475-7516/2011/08/033</dc:relation>
               <dc:relation>info:eu-repo/grantAgreement/EC/FP7/240117/EU//PHYS.LSS</dc:relation>
               <dc:rights>(c) IOP Publishing and Sissa Medialab, 2011</dc:rights>
               <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
               <dc:publisher>Institute of Physics (IOP)</dc:publisher>
               <dc:source>Articles publicats en revistes (Institut de Ciències del Cosmos (ICCUB))</dc:source>
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