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   <dc:title>Non-Gaussian halo assembly bias</dc:title>
   <dc:creator>Reid, Beth A.</dc:creator>
   <dc:creator>Verde, Licia</dc:creator>
   <dc:creator>Dolag, Klaus</dc:creator>
   <dc:creator>Matarrese, Sabino</dc:creator>
   <dc:creator>Moscardini, Lauro</dc:creator>
   <dc:subject>Cosmologia</dc:subject>
   <dc:subject>Astrofísica</dc:subject>
   <dc:subject>Cosmology</dc:subject>
   <dc:subject>Astrophysics</dc:subject>
   <dcterms:abstract>The strong dependence of the large-scale dark matter halo bias on the (local) non-Gaussianity parameter, fNL, offers a promising avenue towards constraining primordial non-Gaussianity with large-scale structure surveys. In this paper, we present the first detection of the dependence of the non-Gaussian halo bias on halo formation history using N-body simulations. We also present an analytic derivation of the expected signal based on the extended Press-Schechter formalism. In excellent agreement with our analytic prediction, we find that the halo formation history-dependent contribution to the non-Gaussian halo bias (which we call non-Gaussian halo assembly bias) can be factorized in a form approximately independent of redshift and halo mass. The correction to the non-Gaussian halo bias due to the halo formation history can be as large as 100%, with a suppression of the signal for recently formed halos and enhancement for old halos. This could in principle be a problem for realistic galaxy surveys if observational selection effects were to pick galaxies occupying only recently formed halos. Current semi-analytic galaxy formation models, for example, imply an enhancement in the expected signal of ~ 23% and ~ 48% for galaxies at z = 1 selected by stellar mass and star formation rate, respectively.</dcterms:abstract>
   <dcterms:issued>2019-01-23T10:54:01Z</dcterms:issued>
   <dcterms:issued>2019-01-23T10:54:01Z</dcterms:issued>
   <dcterms:issued>2010</dcterms:issued>
   <dcterms:issued>2019-01-23T10:54:01Z</dcterms:issued>
   <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/10.1088/1475-7516/2010/07/013</dc:relation>
   <dc:relation>Journal of Cosmology and Astroparticle Physics, 2010, vol. 2010, num. 013</dc:relation>
   <dc:relation>https://doi.org/10.1088/1475-7516/2010/07/013</dc:relation>
   <dc:relation>info:eu-repo/grantAgreement/EC/FP7/240117/EU//PHYS.LSS</dc:relation>
   <dc:rights>(c) IOP Publishing and Sissa Medialab, 2010</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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