FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2083643802> ?p ?o ?g. }

• W2083643802 endingPage "203" @default.
• W2083643802 startingPage "189" @default.
• W2083643802 abstract "We present constraints on the cosmological and reionization parameters based on the cumulative mass function of the Ly-α systems. We evaluate the formation rate of bound objects and their cumulative mass function for a class of flat cosmological models with cold dark matter plus cosmological constant or dark energy with constant equation of state encompassing different reionization scenarios and compare it with the cumulative mass function obtained from the Ly-α transmitted flux power spectrum. We find that the analysis of the cumulative mass function of the Ly-α systems indicates a reionization redshift zr=24.2±4 (68% CL) in agreement with the value found on the basis of the WMAP anisotropy measurements, setting constraints on the amplitude of the density contrast, σ8=0.91±0.04 (68% CL), similar to those derived from the X-ray cluster temperature function. Our joint analysis of Ly-α cumulative mass function and WMAP anisotropy measurements shows that the possible current identification of a running of the slope, dns/dlnk≠0, at kp=0.05 Mpc−1 (multipole l≈700) is mainly an effect of the existing degeneracy in the amplitude–slope plane at this scale, the result being consistent with the absence of running, the other constraints based on WMAP data remaining substantially unchanged. Finally, we evaluate the progress on the determination the considered parameters achievable by using the final temperature anisotropy data from WMAP and from the forthcoming Planck satellite that will significantly improve the sensitivity and reliability of these results. This work has been done in the framework of the Planck LFI activities." @default.
• W2083643802 created "2016-06-24" @default.
• W2083643802 creator A5015901761 @default.
• W2083643802 creator A5039994226 @default.
• W2083643802 creator A5045249514 @default.
• W2083643802 date "2004-03-01" @default.
• W2083643802 modified "2023-09-26" @default.
• W2083643802 title "Nonlinear evolution of the cosmological background density field as diagnostic of the cosmological reionization" @default.
• W2083643802 cites W1536031552 @default.
• W2083643802 cites W1576081563 @default.
• W2083643802 cites W1624215812 @default.
• W2083643802 cites W1966702659 @default.
• W2083643802 cites W1984044687 @default.
• W2083643802 cites W1989563518 @default.
• W2083643802 cites W1998577648 @default.
• W2083643802 cites W2003182532 @default.
• W2083643802 cites W2008441954 @default.
• W2083643802 cites W2018950554 @default.
• W2083643802 cites W2024292892 @default.
• W2083643802 cites W2036818875 @default.
• W2083643802 cites W2049351351 @default.
• W2083643802 cites W2076384560 @default.
• W2083643802 cites W2079948254 @default.
• W2083643802 cites W2083352943 @default.
• W2083643802 cites W2087391133 @default.
• W2083643802 cites W2090436090 @default.
• W2083643802 cites W2092618688 @default.
• W2083643802 cites W2110238788 @default.
• W2083643802 cites W2127896663 @default.
• W2083643802 cites W2161641687 @default.
• W2083643802 cites W2163577447 @default.
• W2083643802 cites W2599720466 @default.
• W2083643802 cites W3007754162 @default.
• W2083643802 cites W3105084986 @default.
• W2083643802 cites W3105493825 @default.
• W2083643802 cites W3105591809 @default.
• W2083643802 cites W3106449272 @default.
• W2083643802 doi "https://doi.org/10.1016/j.newast.2003.10.002" @default.
• W2083643802 hasPublicationYear "2004" @default.
• W2083643802 type Work @default.
• W2083643802 sameAs 2083643802 @default.
• W2083643802 citedByCount "3" @default.
• W2083643802 crossrefType "journal-article" @default.
• W2083643802 hasAuthorship W2083643802A5015901761 @default.
• W2083643802 hasAuthorship W2083643802A5039994226 @default.
• W2083643802 hasAuthorship W2083643802A5045249514 @default.
• W2083643802 hasBestOaLocation W20836438022 @default.
• W2083643802 hasConcept C105795698 @default.
• W2083643802 hasConcept C118534291 @default.
• W2083643802 hasConcept C121332964 @default.
• W2083643802 hasConcept C164008634 @default.
• W2083643802 hasConcept C166126730 @default.
• W2083643802 hasConcept C166861157 @default.
• W2083643802 hasConcept C168110828 @default.
• W2083643802 hasConcept C172790937 @default.
• W2083643802 hasConcept C180205008 @default.
• W2083643802 hasConcept C207297109 @default.
• W2083643802 hasConcept C26405456 @default.
• W2083643802 hasConcept C33024259 @default.
• W2083643802 hasConcept C33923547 @default.
• W2083643802 hasConcept C37914503 @default.
• W2083643802 hasConcept C44870925 @default.
• W2083643802 hasConcept C62520636 @default.
• W2083643802 hasConcept C69672822 @default.
• W2083643802 hasConcept C85725439 @default.
• W2083643802 hasConcept C87485669 @default.
• W2083643802 hasConcept C98444146 @default.
• W2083643802 hasConceptScore W2083643802C105795698 @default.
• W2083643802 hasConceptScore W2083643802C118534291 @default.
• W2083643802 hasConceptScore W2083643802C121332964 @default.
• W2083643802 hasConceptScore W2083643802C164008634 @default.
• W2083643802 hasConceptScore W2083643802C166126730 @default.
• W2083643802 hasConceptScore W2083643802C166861157 @default.
• W2083643802 hasConceptScore W2083643802C168110828 @default.
• W2083643802 hasConceptScore W2083643802C172790937 @default.
• W2083643802 hasConceptScore W2083643802C180205008 @default.
• W2083643802 hasConceptScore W2083643802C207297109 @default.
• W2083643802 hasConceptScore W2083643802C26405456 @default.
• W2083643802 hasConceptScore W2083643802C33024259 @default.
• W2083643802 hasConceptScore W2083643802C33923547 @default.
• W2083643802 hasConceptScore W2083643802C37914503 @default.
• W2083643802 hasConceptScore W2083643802C44870925 @default.
• W2083643802 hasConceptScore W2083643802C62520636 @default.
• W2083643802 hasConceptScore W2083643802C69672822 @default.
• W2083643802 hasConceptScore W2083643802C85725439 @default.
• W2083643802 hasConceptScore W2083643802C87485669 @default.
• W2083643802 hasConceptScore W2083643802C98444146 @default.
• W2083643802 hasIssue "3" @default.
• W2083643802 hasLocation W20836438021 @default.
• W2083643802 hasLocation W20836438022 @default.
• W2083643802 hasOpenAccess W2083643802 @default.
• W2083643802 hasPrimaryLocation W20836438021 @default.
• W2083643802 hasRelatedWork W1546661870 @default.
• W2083643802 hasRelatedWork W1891344458 @default.
• W2083643802 hasRelatedWork W2012342470 @default.
• W2083643802 hasRelatedWork W2888615400 @default.
• W2083643802 hasRelatedWork W2898174274 @default.
• W2083643802 hasRelatedWork W3106220028 @default.

• next