FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2009424252> ?p ?o ?g. }

• W2009424252 endingPage "1010" @default.
• W2009424252 startingPage "994" @default.
• W2009424252 abstract "We use 211 galaxy spectra from our survey for Lyman break galaxies (LBGs) associated with 11 damped Lyα systems (DLAs) to measure the three-dimensional LBG autocorrelation and DLA-LBG cross-correlation functions with the primary goal of inferring the mass of DLAs at z ~ 3. From every measurement and test in this work, we find evidence for an overdensity of LBGs near DLAs that is very similar to that of LBGs near other LBGs. Conventional binning of the data while varying both r0 and γ parameters of the fiducial model of the correlation function ξ(r) = (r/r0)-γ resulted in the best-fit values and 1 σ uncertainties of r0 = 2.65 ± 0.48, γ = 1.55 ± 0.40 for the LBG autocorrelation, and r0 = 3.32 ± 1.25, γ = 1.74 ± 0.36 for the DLA-LBG cross-correlation function. To circumvent shortcomings found in binning small data sets, we perform a maximum likelihood analysis based on Poisson statistics. The best-fit values and 1 σ confidence levels were found to be r0 = 2.91, γ = 1.21 for the LBG autocorrelation, and r0 = 2.81, γ = 2.11 for the DLA-LBG cross-correlation function. We report a redshift spike of five LBGs with Δz = 0.015 of the z = 2.936 DLA in the PSS 0808+5215 field; the DLA-LBG clustering signal survives when omitting this field from the analysis. Using the correlation function measurements and uncertainties, we compute the z ~ 3 LBG galaxy bias bLBG to be 1.5 < bLBG < 3, corresponding to an average halo mass of 109.7 < ⟨MLBG⟩ < 1011.6 M☉, and the z ~ 3 DLA galaxy bias bDLA to be 1.3 < bDLA < 4, corresponding to an average halo mass of 109 < ⟨MLBG⟩ < 1012 M☉. Finally, two of the six QSOs discovered were found to lie within Δz = 0.0125 of two of the survey DLAs. We estimate that the probability of this occurring by chance is 1 in 940, indicating a possible relationship between the distribution of QSOs and DLAs at z ~ 3." @default.
• W2009424252 created "2016-06-24" @default.
• W2009424252 creator A5037615659 @default.
• W2009424252 creator A5046442252 @default.
• W2009424252 creator A5077555623 @default.
• W2009424252 creator A5085250575 @default.
• W2009424252 date "2006-12-01" @default.
• W2009424252 modified "2023-10-18" @default.
• W2009424252 title "Survey for Galaxies Associated with<i>z</i>∼ 3 Damped Lyα Systems. II. Galaxy‐Absorber Correlation Functions" @default.
• W2009424252 cites W1538744062 @default.
• W2009424252 cites W1589711989 @default.
• W2009424252 cites W1637748364 @default.
• W2009424252 cites W1745134529 @default.
• W2009424252 cites W1971343676 @default.
• W2009424252 cites W1972346442 @default.
• W2009424252 cites W1974249877 @default.
• W2009424252 cites W1981769908 @default.
• W2009424252 cites W1981780603 @default.
• W2009424252 cites W1982533357 @default.
• W2009424252 cites W1995229155 @default.
• W2009424252 cites W1995333740 @default.
• W2009424252 cites W1997395325 @default.
• W2009424252 cites W2001490443 @default.
• W2009424252 cites W2004491479 @default.
• W2009424252 cites W2005051185 @default.
• W2009424252 cites W2006189395 @default.
• W2009424252 cites W2006703260 @default.
• W2009424252 cites W2013270856 @default.
• W2009424252 cites W2017047032 @default.
• W2009424252 cites W2020863669 @default.
• W2009424252 cites W2021236310 @default.
• W2009424252 cites W2025634246 @default.
• W2009424252 cites W2027591012 @default.
• W2009424252 cites W2027713091 @default.
• W2009424252 cites W2027853243 @default.
• W2009424252 cites W2029391252 @default.
• W2009424252 cites W2044093857 @default.
• W2009424252 cites W2047247728 @default.
• W2009424252 cites W2048623741 @default.
• W2009424252 cites W2052315062 @default.
• W2009424252 cites W2058379288 @default.
• W2009424252 cites W2059511259 @default.
• W2009424252 cites W2059903494 @default.
• W2009424252 cites W2064662554 @default.
• W2009424252 cites W2083115583 @default.
• W2009424252 cites W2083574565 @default.
• W2009424252 cites W2085479846 @default.
• W2009424252 cites W2086014825 @default.
• W2009424252 cites W2087460385 @default.
• W2009424252 cites W2090894327 @default.
• W2009424252 cites W2094993922 @default.
• W2009424252 cites W2105899817 @default.
• W2009424252 cites W2117105462 @default.
• W2009424252 cites W2154822740 @default.
• W2009424252 cites W2170924363 @default.
• W2009424252 cites W2518704580 @default.
• W2009424252 cites W2951385617 @default.
• W2009424252 cites W3101620743 @default.
• W2009424252 cites W3102200169 @default.
• W2009424252 cites W3102483686 @default.
• W2009424252 cites W3102518111 @default.
• W2009424252 cites W3105230740 @default.
• W2009424252 cites W3106003577 @default.
• W2009424252 cites W3121970673 @default.
• W2009424252 cites W3122244790 @default.
• W2009424252 cites W3123697739 @default.
• W2009424252 cites W3125838123 @default.
• W2009424252 cites W4292508449 @default.
• W2009424252 cites W4292930832 @default.
• W2009424252 doi "https://doi.org/10.1086/507476" @default.
• W2009424252 hasPublicationYear "2006" @default.
• W2009424252 type Work @default.
• W2009424252 sameAs 2009424252 @default.
• W2009424252 citedByCount "65" @default.
• W2009424252 countsByYear W20094242522012 @default.
• W2009424252 countsByYear W20094242522013 @default.
• W2009424252 countsByYear W20094242522014 @default.
• W2009424252 countsByYear W20094242522015 @default.
• W2009424252 countsByYear W20094242522016 @default.
• W2009424252 countsByYear W20094242522017 @default.
• W2009424252 countsByYear W20094242522018 @default.
• W2009424252 countsByYear W20094242522019 @default.
• W2009424252 countsByYear W20094242522020 @default.
• W2009424252 countsByYear W20094242522023 @default.
• W2009424252 crossrefType "journal-article" @default.
• W2009424252 hasAuthorship W2009424252A5037615659 @default.
• W2009424252 hasAuthorship W2009424252A5046442252 @default.
• W2009424252 hasAuthorship W2009424252A5077555623 @default.
• W2009424252 hasAuthorship W2009424252A5085250575 @default.
• W2009424252 hasBestOaLocation W20094242521 @default.
• W2009424252 hasConcept C105795698 @default.
• W2009424252 hasConcept C121332964 @default.
• W2009424252 hasConcept C133386390 @default.
• W2009424252 hasConcept C184665706 @default.
• W2009424252 hasConcept C33024259 @default.
• W2009424252 hasConcept C33923547 @default.
• W2009424252 hasConcept C44870925 @default.
• W2009424252 hasConcept C5297727 @default.

• next