FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2074037441> ?p ?o ?g. }

• W2074037441 endingPage "803" @default.
• W2074037441 startingPage "778" @default.
• W2074037441 abstract "We use the deep ground-based optical photometry of the Lyman Break Galaxy (LBG) Survey to derive robust measurements of the faint-end slope (alpha) of the UV LF at redshifts 1.9<z<3.4. Our sample includes >2000 spectroscopic redshifts and ~31000 LBGs in 31 spatially-independent fields over a total area of 3261 arcmin^2. These data allow us to select galaxies to 0.07L* and 0.10L* at z~2 and z~3, respectively. A maximum likelihood analysis indicates steep values of alpha(z=2)=-1.73+/-0.07 and alpha(z=3)=-1.73+/-0.13. This result is robust to luminosity dependent systematics in the Ly-alpha equivalent width and reddening distributions, is similar to the steep values advocated at z>4, and implies that ~93% of the unobscured UV luminosity density at z~2-3 arises from sub-L* galaxies. With a realistic luminosity dependent reddening distribution, faint to moderately luminous galaxies account for >70% and >25% of the bolometric luminosity density and present-day stellar mass density, respectively, when integrated over 1.9<z<3.4. We find a factor of 8-9 increase in the star formation rate density between z~6 and z~2, due to both a brightening of L* and an increasing dust correction proceeding to lower redshifts. The previously observed discrepancy between the integral of the star formation history and stellar mass density measurements at z~2 may be reconciled by invoking a luminosity dependent reddening correction to the star formation history combined with an accounting for the stellar mass contributed by UV-faint galaxies. The steep and relatively constant alpha of the UV LF at z>2 contrasts with the shallower value inferred locally, suggesting that the evolution in the faint-end slope may be dictated simply by the availability of low mass halos capable of supporting star formation at z<2. [Abridged]" @default.
• W2074037441 created "2016-06-24" @default.
• W2074037441 creator A5028023592 @default.
• W2074037441 creator A5057083130 @default.
• W2074037441 date "2009-02-10" @default.
• W2074037441 modified "2023-10-13" @default.
• W2074037441 title "A STEEP FAINT-END SLOPE OF THE UV LUMINOSITY FUNCTION AT<i>z</i>∼ 2-3: IMPLICATIONS FOR THE GLOBAL STELLAR MASS DENSITY AND STAR FORMATION IN LOW-MASS HALOS" @default.
• W2074037441 cites W1484400061 @default.
• W2074037441 cites W1607434071 @default.
• W2074037441 cites W1622230873 @default.
• W2074037441 cites W1681063222 @default.
• W2074037441 cites W1964344398 @default.
• W2074037441 cites W1965779302 @default.
• W2074037441 cites W1969214334 @default.
• W2074037441 cites W1972507852 @default.
• W2074037441 cites W1973977373 @default.
• W2074037441 cites W1983192361 @default.
• W2074037441 cites W1988697524 @default.
• W2074037441 cites W1994033192 @default.
• W2074037441 cites W1994671833 @default.
• W2074037441 cites W2000126425 @default.
• W2074037441 cites W2006316173 @default.
• W2074037441 cites W2007741717 @default.
• W2074037441 cites W2007775671 @default.
• W2074037441 cites W2012035798 @default.
• W2074037441 cites W2012886609 @default.
• W2074037441 cites W2012983802 @default.
• W2074037441 cites W2013375438 @default.
• W2074037441 cites W2014203224 @default.
• W2074037441 cites W2015295900 @default.
• W2074037441 cites W2015529116 @default.
• W2074037441 cites W2016766153 @default.
• W2074037441 cites W2016966639 @default.
• W2074037441 cites W2017047032 @default.
• W2074037441 cites W2017100570 @default.
• W2074037441 cites W2020863669 @default.
• W2074037441 cites W2023270129 @default.
• W2074037441 cites W2023573418 @default.
• W2074037441 cites W2024297548 @default.
• W2074037441 cites W2025078251 @default.
• W2074037441 cites W2025458316 @default.
• W2074037441 cites W2025913857 @default.
• W2074037441 cites W2028508207 @default.
• W2074037441 cites W2029466024 @default.
• W2074037441 cites W2037929101 @default.
• W2074037441 cites W2039833992 @default.
• W2074037441 cites W2040441522 @default.
• W2074037441 cites W2043038124 @default.
• W2074037441 cites W2046338642 @default.
• W2074037441 cites W2052315062 @default.
• W2074037441 cites W2053321229 @default.
• W2074037441 cites W2054851301 @default.
• W2074037441 cites W2059037849 @default.
• W2074037441 cites W2066702052 @default.
• W2074037441 cites W2066849118 @default.
• W2074037441 cites W2068368465 @default.
• W2074037441 cites W2070696493 @default.
• W2074037441 cites W2075105252 @default.
• W2074037441 cites W2077537026 @default.
• W2074037441 cites W2081243021 @default.
• W2074037441 cites W2083365390 @default.
• W2074037441 cites W2084830951 @default.
• W2074037441 cites W2091867375 @default.
• W2074037441 cites W2093340168 @default.
• W2074037441 cites W2093468672 @default.
• W2074037441 cites W2098171023 @default.
• W2074037441 cites W2098914923 @default.
• W2074037441 cites W2101058963 @default.
• W2074037441 cites W2114951275 @default.
• W2074037441 cites W2118572026 @default.
• W2074037441 cites W2124572431 @default.
• W2074037441 cites W2125977823 @default.
• W2074037441 cites W2129760210 @default.
• W2074037441 cites W2131053676 @default.
• W2074037441 cites W2131462302 @default.
• W2074037441 cites W2137987137 @default.
• W2074037441 cites W2138587471 @default.
• W2074037441 cites W2140887005 @default.
• W2074037441 cites W2142238829 @default.
• W2074037441 cites W2146103050 @default.
• W2074037441 cites W2150995848 @default.
• W2074037441 cites W2151062050 @default.
• W2074037441 cites W2154748230 @default.
• W2074037441 cites W2155805383 @default.
• W2074037441 cites W2162516451 @default.
• W2074037441 cites W2164106029 @default.
• W2074037441 cites W2166026900 @default.
• W2074037441 cites W2169075455 @default.
• W2074037441 cites W2315647678 @default.
• W2074037441 cites W2330599159 @default.
• W2074037441 cites W2950611332 @default.
• W2074037441 cites W2951752678 @default.
• W2074037441 cites W3099302206 @default.
• W2074037441 cites W3099471130 @default.
• W2074037441 cites W3100787184 @default.
• W2074037441 cites W3100949304 @default.
• W2074037441 cites W3100987540 @default.
• W2074037441 cites W3101282852 @default.

• next