FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3106346350> ?p ?o ?g. }

• W3106346350 endingPage "1256" @default.
• W3106346350 startingPage "1244" @default.
• W3106346350 abstract "We present measurements of the clustering properties of bright (L > L*) z~4 Lyman break galaxies (LBGs) selected from the Oxford-Dartmouth Thirty Degree Survey (ODT). We describe techniques used to select and evaluate our candidates and calculate the angular correlation function, which we find best fitted by a power law, ω(θ) =Awθ−β with Aw= 15.4 (with θ in arcsec), using a constrained slope of β= 0.8. Using a redshift distribution consistent with photometric models, we deproject this correlation function and find a comoving Mpc in a Ωm= 0.3 flat λ cosmology for iAB≤ 24.5. This corresponds to a linear bias value of (assuming σ8= 0.9). These data show a significantly larger r0 and b than previous studies at z~4. We interpret this as evidence that the brightest LBGs have a larger bias than fainter ones, indicating a strong luminosity dependence for the measured bias of an LBG sample. Comparing this against recent results in the literature at fainter (subL*) limiting magnitudes, and with simple models describing the relationship between LBGs and dark matter haloes, we discuss the implications on the implied environments and nature of LBGs. It seems that the brightest LBGs (in contrast with the majority subL* population) have clustering properties, and host dark matter halo masses, which are consistent with them being progenitors of the most massive galaxies today." @default.
• W3106346350 created "2020-11-23" @default.
• W3106346350 creator A5011140827 @default.
• W3106346350 creator A5014464961 @default.
• W3106346350 creator A5015312473 @default.
• W3106346350 creator A5040323320 @default.
• W3106346350 creator A5056209660 @default.
• W3106346350 creator A5078232830 @default.
• W3106346350 creator A5084029871 @default.
• W3106346350 creator A5088379970 @default.
• W3106346350 date "2005-07-01" @default.
• W3106346350 modified "2023-10-06" @default.
• W3106346350 title "The Oxford-Dartmouth Thirty Degree Survey - II. Clustering of bright Lyman break galaxies: strong luminosity-dependent bias at<i>z</i>= 4" @default.
• W3106346350 cites W1965779302 @default.
• W3106346350 cites W1974159111 @default.
• W3106346350 cites W1984336612 @default.
• W3106346350 cites W1993856735 @default.
• W3106346350 cites W1996976369 @default.
• W3106346350 cites W1998961346 @default.
• W3106346350 cites W2001373670 @default.
• W3106346350 cites W2010395680 @default.
• W3106346350 cites W2012056991 @default.
• W3106346350 cites W2015233984 @default.
• W3106346350 cites W2018148195 @default.
• W3106346350 cites W2021719201 @default.
• W3106346350 cites W2025634246 @default.
• W3106346350 cites W2029923300 @default.
• W3106346350 cites W2030154533 @default.
• W3106346350 cites W2030612271 @default.
• W3106346350 cites W2034244568 @default.
• W3106346350 cites W2043546334 @default.
• W3106346350 cites W2044989646 @default.
• W3106346350 cites W2052315062 @default.
• W3106346350 cites W2057490476 @default.
• W3106346350 cites W2057672934 @default.
• W3106346350 cites W2058730141 @default.
• W3106346350 cites W2059511259 @default.
• W3106346350 cites W2060908453 @default.
• W3106346350 cites W2075400007 @default.
• W3106346350 cites W2082012530 @default.
• W3106346350 cites W2082266584 @default.
• W3106346350 cites W2095855161 @default.
• W3106346350 cites W2101739777 @default.
• W3106346350 cites W2114951275 @default.
• W3106346350 cites W2116625717 @default.
• W3106346350 cites W2117498035 @default.
• W3106346350 cites W2121712078 @default.
• W3106346350 cites W2126711037 @default.
• W3106346350 cites W2134712793 @default.
• W3106346350 cites W2142238829 @default.
• W3106346350 cites W2153106528 @default.
• W3106346350 cites W2155711232 @default.
• W3106346350 cites W2518704580 @default.
• W3106346350 cites W2950115961 @default.
• W3106346350 cites W2951752678 @default.
• W3106346350 cites W3098017603 @default.
• W3106346350 cites W3099710293 @default.
• W3106346350 cites W3100669571 @default.
• W3106346350 cites W3101247804 @default.
• W3106346350 cites W3101620743 @default.
• W3106346350 cites W3102483686 @default.
• W3106346350 cites W3103271964 @default.
• W3106346350 cites W3106003577 @default.
• W3106346350 cites W3106491886 @default.
• W3106346350 cites W3106526798 @default.
• W3106346350 cites W3122244790 @default.
• W3106346350 cites W4243734499 @default.
• W3106346350 cites W4292508449 @default.
• W3106346350 cites W4298856267 @default.
• W3106346350 cites W4300521843 @default.
• W3106346350 doi "https://doi.org/10.1111/j.1365-2966.2005.09161.x" @default.
• W3106346350 hasPublicationYear "2005" @default.
• W3106346350 type Work @default.
• W3106346350 sameAs 3106346350 @default.
• W3106346350 citedByCount "28" @default.
• W3106346350 countsByYear W31063463502015 @default.
• W3106346350 countsByYear W31063463502017 @default.
• W3106346350 countsByYear W31063463502018 @default.
• W3106346350 crossrefType "journal-article" @default.
• W3106346350 hasAuthorship W3106346350A5011140827 @default.
• W3106346350 hasAuthorship W3106346350A5014464961 @default.
• W3106346350 hasAuthorship W3106346350A5015312473 @default.
• W3106346350 hasAuthorship W3106346350A5040323320 @default.
• W3106346350 hasAuthorship W3106346350A5056209660 @default.
• W3106346350 hasAuthorship W3106346350A5078232830 @default.
• W3106346350 hasAuthorship W3106346350A5084029871 @default.
• W3106346350 hasAuthorship W3106346350A5088379970 @default.
• W3106346350 hasBestOaLocation W31063463501 @default.
• W3106346350 hasConcept C105795698 @default.
• W3106346350 hasConcept C121332964 @default.
• W3106346350 hasConcept C12287442 @default.
• W3106346350 hasConcept C1276947 @default.
• W3106346350 hasConcept C133386390 @default.
• W3106346350 hasConcept C144024400 @default.
• W3106346350 hasConcept C149923435 @default.
• W3106346350 hasConcept C159249277 @default.
• W3106346350 hasConcept C17959413 @default.
• W3106346350 hasConcept C184665706 @default.

• next