FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2079222316> ?p ?o ?g. }

• W2079222316 abstract "We use measurements of luminosity-dependent galaxy bias at several different redshifts, SDSS at $z=0.05$, DEEP2 at $z=1$, and LBGs at $z=3.8$, combined with WMAP 5-year cosmic microwave background anisotropy data and SDSS Red Luminous Galaxy survey three-dimensional clustering power spectrum to put constraints on cosmological parameters. Fitting this combined dataset, we show that the luminosity-dependent bias data that probe the relation between halo bias and halo mass and its redshift evolution are very sensitive to sum of the neutrino masses: in particular, we obtain the upper limit of $ensuremath{sum}_{}^{}{m}_{ensuremath{nu}}<0.28text{ }text{ }mathrm{eV}$ at the 95% confidence level for a $ensuremath{Lambda}mathrm{CDM}+{m}_{ensuremath{nu}}$ model, with a ${ensuremath{sigma}}_{8}$ equal to ${ensuremath{sigma}}_{8}=0.759ifmmodepmelsetextpmfi{}0.025$ ($1ensuremath{sigma}$). When we allow the dark energy equation-of-state parameter $w$ to vary, we find $w=ensuremath{-}1.30ifmmodepmelsetextpmfi{}0.19$ for a general $wmathrm{CDM}+{m}_{ensuremath{nu}}$ model with the 95% confidence level upper limit on the neutrino masses at $ensuremath{sum}_{}^{}{m}_{ensuremath{nu}}<0.59text{ }text{ }mathrm{eV}$. The constraint on the dark energy equation of state further improves to $w=ensuremath{-}1.125ifmmodepmelsetextpmfi{}0.092$ when using also ACBAR and supernovae Union data, in addition to above, with a prior on the Hubble constant from the Hubble Space Telescope." @default.
• W2079222316 created "2016-06-24" @default.
• W2079222316 creator A5015735436 @default.
• W2079222316 creator A5016781401 @default.
• W2079222316 creator A5072280155 @default.
• W2079222316 creator A5082121413 @default.
• W2079222316 date "2008-10-24" @default.
• W2079222316 modified "2023-09-28" @default.
• W2079222316 title "Improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-break galaxies" @default.
• W2079222316 cites W1498004781 @default.
• W2079222316 cites W1506722212 @default.
• W2079222316 cites W1529115508 @default.
• W2079222316 cites W1765639848 @default.
• W2079222316 cites W1894431533 @default.
• W2079222316 cites W1959064610 @default.
• W2079222316 cites W1965779302 @default.
• W2079222316 cites W1971757169 @default.
• W2079222316 cites W1972662854 @default.
• W2079222316 cites W1978425005 @default.
• W2079222316 cites W1982533357 @default.
• W2079222316 cites W1983915301 @default.
• W2079222316 cites W1991618825 @default.
• W2079222316 cites W1996378698 @default.
• W2079222316 cites W1998731207 @default.
• W2079222316 cites W2000310419 @default.
• W2079222316 cites W2002142654 @default.
• W2079222316 cites W2006189395 @default.
• W2079222316 cites W2014203171 @default.
• W2079222316 cites W2018719255 @default.
• W2079222316 cites W2023068686 @default.
• W2079222316 cites W2035000458 @default.
• W2079222316 cites W2044117497 @default.
• W2079222316 cites W2061899254 @default.
• W2079222316 cites W2070550349 @default.
• W2079222316 cites W2088172914 @default.
• W2079222316 cites W2121991715 @default.
• W2079222316 cites W2126510815 @default.
• W2079222316 cites W2131260550 @default.
• W2079222316 cites W2139440433 @default.
• W2079222316 cites W2139900404 @default.
• W2079222316 cites W2144924365 @default.
• W2079222316 cites W2147431302 @default.
• W2079222316 cites W2148534890 @default.
• W2079222316 cites W2150904269 @default.
• W2079222316 cites W2151761100 @default.
• W2079222316 cites W2153208487 @default.
• W2079222316 cites W2153811626 @default.
• W2079222316 cites W2157544440 @default.
• W2079222316 cites W3099875550 @default.
• W2079222316 cites W3101168514 @default.
• W2079222316 cites W3102987263 @default.
• W2079222316 cites W3103838041 @default.
• W2079222316 cites W3104206851 @default.
• W2079222316 cites W3104639138 @default.
• W2079222316 cites W3104746642 @default.
• W2079222316 cites W3105554724 @default.
• W2079222316 cites W3105631369 @default.
• W2079222316 cites W3106195644 @default.
• W2079222316 cites W4243734499 @default.
• W2079222316 doi "https://doi.org/10.1103/physrevd.78.083535" @default.
• W2079222316 hasPublicationYear "2008" @default.
• W2079222316 type Work @default.
• W2079222316 sameAs 2079222316 @default.
• W2079222316 citedByCount "22" @default.
• W2079222316 countsByYear W20792223162012 @default.
• W2079222316 countsByYear W20792223162014 @default.
• W2079222316 countsByYear W20792223162015 @default.
• W2079222316 countsByYear W20792223162019 @default.
• W2079222316 crossrefType "journal-article" @default.
• W2079222316 hasAuthorship W2079222316A5015735436 @default.
• W2079222316 hasAuthorship W2079222316A5016781401 @default.
• W2079222316 hasAuthorship W2079222316A5072280155 @default.
• W2079222316 hasAuthorship W2079222316A5082121413 @default.
• W2079222316 hasBestOaLocation W20792223162 @default.
• W2079222316 hasConcept C103874350 @default.
• W2079222316 hasConcept C109214941 @default.
• W2079222316 hasConcept C121332964 @default.
• W2079222316 hasConcept C12287442 @default.
• W2079222316 hasConcept C172790937 @default.
• W2079222316 hasConcept C184665706 @default.
• W2079222316 hasConcept C186453547 @default.
• W2079222316 hasConcept C207297109 @default.
• W2079222316 hasConcept C26405456 @default.
• W2079222316 hasConcept C2779770503 @default.
• W2079222316 hasConcept C33024259 @default.
• W2079222316 hasConcept C44870925 @default.
• W2079222316 hasConcept C62520636 @default.
• W2079222316 hasConcept C85725439 @default.
• W2079222316 hasConcept C87485669 @default.
• W2079222316 hasConcept C98444146 @default.
• W2079222316 hasConceptScore W2079222316C103874350 @default.
• W2079222316 hasConceptScore W2079222316C109214941 @default.
• W2079222316 hasConceptScore W2079222316C121332964 @default.
• W2079222316 hasConceptScore W2079222316C12287442 @default.
• W2079222316 hasConceptScore W2079222316C172790937 @default.
• W2079222316 hasConceptScore W2079222316C184665706 @default.
• W2079222316 hasConceptScore W2079222316C186453547 @default.
• W2079222316 hasConceptScore W2079222316C207297109 @default.
• W2079222316 hasConceptScore W2079222316C26405456 @default.
• W2079222316 hasConceptScore W2079222316C2779770503 @default.

• next