FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100017710> ?p ?o ?g. }

• W3100017710 endingPage "91" @default.
• W3100017710 startingPage "91" @default.
• W3100017710 abstract "The properties of submillimeter galaxies (SMGs) that are fainter than the confusion limit of blank-field single-dish surveys ($S_{850} lesssim$ 2 mJy) are poorly constrained. Using a newly developed color selection technique, Optical-Infrared Triple Color (OIRTC), that has been shown to successfully {select} such faint SMGs, we identify a sample of 2938 OIRTC-selected galaxies, dubbed Triple Color Galaxies (TCGs), in the UKIDSS-UDS field. We show that these galaxies have a median 850 $mu$m flux of S$_{850} = 0.96pm0.04$ mJy (equivalent to a star-formation rate SFR $sim60-100$ M$_odot$ yr$^{-1}$ based on SED fitting), representing the first large sample of faint SMGs that bridges the gap between bright SMGs and normal star-forming galaxies in S$_{850}$ and $L_{rm IR}$. We assess the basic properties of TCGs and their relationship with other galaxy populations at $zsim2$. We measure the two-point autocorrelation function for this population and derive a typical halo mass of log$_{10}$(M$_{rm halo}$) $=12.9^{+0.2}_{-0.3}$, $12.7^{+0.1}_{-0.2}$, and $12.9^{+0.2}_{-0.3}$ $h^{-1}$M$_odot$ at $z=1-2$, $2-3$, and $3-5$, respectively. Together with the bright SMGs (S$_{850} gtrsim 2$ mJy) and a comparison sample of less far-infrared luminous star-forming galaxies, we find a lack of dependence between spatial clustering and S$_{850}$ (or SFR), suggesting that the difference between these populations may lie in their local galactic environment. Lastly, on the scale of $sim8-17$ kpc at $1<z<5$ we find a tentative enhancement of the clustering of TCGs over the comparison star-forming galaxies, suggesting that some faint SMGs are physically associated pairs, perhaps reflecting a merging origin in their triggering." @default.
• W3100017710 created "2020-11-23" @default.
• W3100017710 creator A5000559800 @default.
• W3100017710 creator A5033156566 @default.
• W3100017710 creator A5034769481 @default.
• W3100017710 creator A5035445329 @default.
• W3100017710 creator A5039267303 @default.
• W3100017710 creator A5040248059 @default.
• W3100017710 creator A5048707483 @default.
• W3100017710 creator A5061458577 @default.
• W3100017710 creator A5063774673 @default.
• W3100017710 creator A5079292325 @default.
• W3100017710 date "2016-10-28" @default.
• W3100017710 modified "2023-09-25" @default.
• W3100017710 title "FAINT SUBMILLIMETER GALAXIES IDENTIFIED THROUGH THEIR OPTICAL/NEAR-INFRARED COLORS. I. SPATIAL CLUSTERING AND HALO MASSES" @default.
• W3100017710 cites W1668717269 @default.
• W3100017710 cites W1925976652 @default.
• W3100017710 cites W1929330687 @default.
• W3100017710 cites W1948197607 @default.
• W3100017710 cites W1965166314 @default.
• W3100017710 cites W1970196846 @default.
• W3100017710 cites W1972053729 @default.
• W3100017710 cites W1982533357 @default.
• W3100017710 cites W1983114396 @default.
• W3100017710 cites W1986738273 @default.
• W3100017710 cites W1987592311 @default.
• W3100017710 cites W1989236130 @default.
• W3100017710 cites W1991171205 @default.
• W3100017710 cites W1994671833 @default.
• W3100017710 cites W1996990154 @default.
• W3100017710 cites W2003123765 @default.
• W3100017710 cites W2013964487 @default.
• W3100017710 cites W2014651197 @default.
• W3100017710 cites W2015761009 @default.
• W3100017710 cites W2017047032 @default.
• W3100017710 cites W2017100570 @default.
• W3100017710 cites W2018719255 @default.
• W3100017710 cites W2020084262 @default.
• W3100017710 cites W2021277919 @default.
• W3100017710 cites W2024409675 @default.
• W3100017710 cites W2025105301 @default.
• W3100017710 cites W2025634246 @default.
• W3100017710 cites W2028398011 @default.
• W3100017710 cites W2028626541 @default.
• W3100017710 cites W2037572085 @default.
• W3100017710 cites W2040520625 @default.
• W3100017710 cites W2045977584 @default.
• W3100017710 cites W2051291450 @default.
• W3100017710 cites W2053682218 @default.
• W3100017710 cites W2055864709 @default.
• W3100017710 cites W2060572005 @default.
• W3100017710 cites W2064998288 @default.
• W3100017710 cites W2073193582 @default.
• W3100017710 cites W2073925265 @default.
• W3100017710 cites W2074106980 @default.
• W3100017710 cites W2078441390 @default.
• W3100017710 cites W2079304679 @default.
• W3100017710 cites W2082592033 @default.
• W3100017710 cites W2082674267 @default.
• W3100017710 cites W2082727428 @default.
• W3100017710 cites W2084699143 @default.
• W3100017710 cites W2090459210 @default.
• W3100017710 cites W2093117272 @default.
• W3100017710 cites W2093468672 @default.
• W3100017710 cites W2094504621 @default.
• W3100017710 cites W2098097810 @default.
• W3100017710 cites W2116466430 @default.
• W3100017710 cites W2117363750 @default.
• W3100017710 cites W2117885077 @default.
• W3100017710 cites W2123709957 @default.
• W3100017710 cites W2124602325 @default.
• W3100017710 cites W2135052708 @default.
• W3100017710 cites W2135625048 @default.
• W3100017710 cites W2139937287 @default.
• W3100017710 cites W2142238829 @default.
• W3100017710 cites W2155078682 @default.
• W3100017710 cites W2160156500 @default.
• W3100017710 cites W2162596494 @default.
• W3100017710 cites W2165924595 @default.
• W3100017710 cites W2167009888 @default.
• W3100017710 cites W2168035859 @default.
• W3100017710 cites W2168126149 @default.
• W3100017710 cites W2171300221 @default.
• W3100017710 cites W2171845096 @default.
• W3100017710 cites W2197026494 @default.
• W3100017710 cites W2213987980 @default.
• W3100017710 cites W2226025607 @default.
• W3100017710 cites W2237129515 @default.
• W3100017710 cites W2261374016 @default.
• W3100017710 cites W2345726238 @default.
• W3100017710 cites W2949874561 @default.
• W3100017710 cites W2950611332 @default.
• W3100017710 cites W3098220822 @default.
• W3100017710 cites W3098339022 @default.
• W3100017710 cites W3098540562 @default.
• W3100017710 cites W3098561127 @default.
• W3100017710 cites W3099172813 @default.
• W3100017710 cites W3099267591 @default.

• next