FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2059635105> ?p ?o ?g. }

• W2059635105 endingPage "018" @default.
• W2059635105 startingPage "018" @default.
• W2059635105 abstract "The cross-correlation between cosmic microwave background (CMB) temperature anisotropies and the large-scale structure (LSS) traced by the galaxy distribution, or sources at different wavelengths, is now well known. This correlation results from the integrated Sachs–Wolfe (ISW) effect in CMB anisotropies generated at late times due to the dark energy component of the Universe. In a reionized universe, electron scattering at low redshifts leads to a large-scale polarization contribution. In addition to the primordial quadrupole, involving anisotropies at the last scattering surface, the ISW quadrupole rescatters and contributes to the large angular scale polarization signal. Thus, in principle, the low multipole polarization bump in the E-mode should be correlated with the galaxy distribution. Unlike the CMB temperature–LSS correlation that peaks for tracers at low redshifts, due to the increasing visibility function, while the fractional ISW quadrupole is decreasing, with increasing redshift, the polarization–galaxy correlation peaks mostly at redshifts between 1 and 3. Under certain conditions, mostly involving a low optical depth to reionization if the Universe reionized at a redshift around 6, the cross-polarization–source signal is marginally detectable if all-sky maps of the large-scale structure at redshifts between 1 and 3 are available. If the Universe reionized at a redshift higher than 10, it is unlikely that this correlation will be detectable even with no instrumental noise all-sky maps. While our estimates do not guarantee a detection, unknown physics related to the dark energy uncertain issues related to the large angular scale CMB and polarization anisotropies, and uncertainties related to the reionization history of the Universe may motivate attempts to measure this correlation using upcoming CMB polarization E-mode maps and large-scale structure maps of the high-redshift universe with the Large Synoptic Survey Telescope and quasar catalogues, among others." @default.
• W2059635105 created "2016-06-24" @default.
• W2059635105 creator A5016781401 @default.
• W2059635105 creator A5072280155 @default.
• W2059635105 date "2006-01-24" @default.
• W2059635105 modified "2023-10-03" @default.
• W2059635105 title "Searching for integrated Sachs–Wolfe effect beyond temperature anisotropies: CMB E-mode polarization–galaxy cross-correlation" @default.
• W2059635105 cites W1579845354 @default.
• W2059635105 cites W1594622226 @default.
• W2059635105 cites W1839108935 @default.
• W2059635105 cites W1963562648 @default.
• W2059635105 cites W1971340911 @default.
• W2059635105 cites W1980647430 @default.
• W2059635105 cites W1984527122 @default.
• W2059635105 cites W1985909835 @default.
• W2059635105 cites W2013373833 @default.
• W2059635105 cites W2023573336 @default.
• W2059635105 cites W2023966254 @default.
• W2059635105 cites W2037412966 @default.
• W2059635105 cites W2050277935 @default.
• W2059635105 cites W2050865352 @default.
• W2059635105 cites W2053613213 @default.
• W2059635105 cites W2070430980 @default.
• W2059635105 cites W2083051218 @default.
• W2059635105 cites W2089757105 @default.
• W2059635105 cites W2118265220 @default.
• W2059635105 cites W2122531913 @default.
• W2059635105 cites W2126158412 @default.
• W2059635105 cites W2135040130 @default.
• W2059635105 cites W2135125956 @default.
• W2059635105 cites W2135636048 @default.
• W2059635105 cites W2137168535 @default.
• W2059635105 cites W2140688245 @default.
• W2059635105 cites W2147396839 @default.
• W2059635105 cites W2168949285 @default.
• W2059635105 cites W2171042027 @default.
• W2059635105 cites W2949296060 @default.
• W2059635105 cites W2951034677 @default.
• W2059635105 cites W3004198491 @default.
• W2059635105 cites W3103580489 @default.
• W2059635105 cites W3121431427 @default.
• W2059635105 doi "https://doi.org/10.1088/1475-7516/2006/01/018" @default.
• W2059635105 hasPublicationYear "2006" @default.
• W2059635105 type Work @default.
• W2059635105 sameAs 2059635105 @default.
• W2059635105 citedByCount "9" @default.
• W2059635105 countsByYear W20596351052016 @default.
• W2059635105 countsByYear W20596351052018 @default.
• W2059635105 crossrefType "journal-article" @default.
• W2059635105 hasAuthorship W2059635105A5016781401 @default.
• W2059635105 hasAuthorship W2059635105A5072280155 @default.
• W2059635105 hasConcept C120665830 @default.
• W2059635105 hasConcept C121332964 @default.
• W2059635105 hasConcept C1276947 @default.
• W2059635105 hasConcept C147789679 @default.
• W2059635105 hasConcept C172790937 @default.
• W2059635105 hasConcept C185592680 @default.
• W2059635105 hasConcept C205049153 @default.
• W2059635105 hasConcept C207297109 @default.
• W2059635105 hasConcept C26405456 @default.
• W2059635105 hasConcept C2779556658 @default.
• W2059635105 hasConcept C33024259 @default.
• W2059635105 hasConcept C44870925 @default.
• W2059635105 hasConcept C56764 @default.
• W2059635105 hasConcept C69672822 @default.
• W2059635105 hasConcept C85725439 @default.
• W2059635105 hasConcept C98444146 @default.
• W2059635105 hasConceptScore W2059635105C120665830 @default.
• W2059635105 hasConceptScore W2059635105C121332964 @default.
• W2059635105 hasConceptScore W2059635105C1276947 @default.
• W2059635105 hasConceptScore W2059635105C147789679 @default.
• W2059635105 hasConceptScore W2059635105C172790937 @default.
• W2059635105 hasConceptScore W2059635105C185592680 @default.
• W2059635105 hasConceptScore W2059635105C205049153 @default.
• W2059635105 hasConceptScore W2059635105C207297109 @default.
• W2059635105 hasConceptScore W2059635105C26405456 @default.
• W2059635105 hasConceptScore W2059635105C2779556658 @default.
• W2059635105 hasConceptScore W2059635105C33024259 @default.
• W2059635105 hasConceptScore W2059635105C44870925 @default.
• W2059635105 hasConceptScore W2059635105C56764 @default.
• W2059635105 hasConceptScore W2059635105C69672822 @default.
• W2059635105 hasConceptScore W2059635105C85725439 @default.
• W2059635105 hasConceptScore W2059635105C98444146 @default.
• W2059635105 hasIssue "01" @default.
• W2059635105 hasLocation W20596351051 @default.
• W2059635105 hasOpenAccess W2059635105 @default.
• W2059635105 hasPrimaryLocation W20596351051 @default.
• W2059635105 hasRelatedWork W2056950111 @default.
• W2059635105 hasRelatedWork W2059635105 @default.
• W2059635105 hasRelatedWork W2198489812 @default.
• W2059635105 hasRelatedWork W2957244501 @default.
• W2059635105 hasRelatedWork W3009121361 @default.
• W2059635105 hasRelatedWork W3098742842 @default.
• W2059635105 hasRelatedWork W3104596674 @default.
• W2059635105 hasRelatedWork W3176532687 @default.
• W2059635105 hasRelatedWork W4299539120 @default.
• W2059635105 hasRelatedWork W2467367807 @default.
• W2059635105 hasVolume "2006" @default.

• next