Matches in SemOpenAlex for { <https://semopenalex.org/work/W3098805361> ?p ?o ?g. }
- W3098805361 endingPage "78" @default.
- W3098805361 startingPage "78" @default.
- W3098805361 abstract "Until recently, only a handful of dusty, star-forming galaxies (DSFGs) were known at $z>4$, most of them significantly amplified by gravitational lensing. Here, we have increased the number of such DSFGs substantially, selecting galaxies from the uniquely wide 250-, 350- and 500-$mu$m Herschel-ATLAS imaging survey on the basis of their extremely red far-infrared colors and faint 350- and 500-$mu$m flux densities - ergo they are expected to be largely unlensed, luminous, rare and very distant. The addition of ground-based continuum photometry at longer wavelengths from the JCMT and APEX allows us to identify the dust peak in their SEDs, better constraining their redshifts. We select the SED templates best able to determine photometric redshifts using a sample of 69 high-redshift, lensed DSFGs, then perform checks to assess the impact of the CMB on our technique, and to quantify the systematic uncertainty associated with our photometric redshifts, $sigma=0.14,(1+z)$, using a sample of 25 galaxies with spectroscopic redshifts, each consistent with our color selection. For Herschel-selected ultrared galaxies with typical colors of $S_{500}/S_{250}sim 2.2$ and $S_{500}/S_{350}sim 1.3$ and flux densities, $S_{500}sim 50,$mJy, we determine a median redshift, $hat{z}_{rm phot}=3.66$, an interquartile redshift range, 3.30$-$4.27, with a median rest-frame 8$-$1000-$mu$m luminosity, $hat{L}_{rm IR}$, of $1.3times 10^{13},$L$_odot$. A third lie at $z>4$, suggesting a space density, $rho_{z>4}$, of $approx 6 times 10^{-7},$Mpc$^{-3}$. Our sample contains the most luminous known star-forming galaxies, and the most over-dense cluster of starbursting proto-ellipticals yet found." @default.
- W3098805361 created "2020-11-23" @default.
- W3098805361 creator A5001581138 @default.
- W3098805361 creator A5003312927 @default.
- W3098805361 creator A5006130261 @default.
- W3098805361 creator A5018789920 @default.
- W3098805361 creator A5019966786 @default.
- W3098805361 creator A5021071629 @default.
- W3098805361 creator A5022805742 @default.
- W3098805361 creator A5024654158 @default.
- W3098805361 creator A5024688962 @default.
- W3098805361 creator A5026859057 @default.
- W3098805361 creator A5026859867 @default.
- W3098805361 creator A5030109075 @default.
- W3098805361 creator A5037826453 @default.
- W3098805361 creator A5040248059 @default.
- W3098805361 creator A5042132634 @default.
- W3098805361 creator A5047609242 @default.
- W3098805361 creator A5048707483 @default.
- W3098805361 creator A5053593436 @default.
- W3098805361 creator A5054140444 @default.
- W3098805361 creator A5060434425 @default.
- W3098805361 creator A5062504729 @default.
- W3098805361 creator A5063774673 @default.
- W3098805361 creator A5064305768 @default.
- W3098805361 creator A5065328861 @default.
- W3098805361 creator A5067446077 @default.
- W3098805361 creator A5069070639 @default.
- W3098805361 creator A5071172705 @default.
- W3098805361 creator A5072280155 @default.
- W3098805361 creator A5073786396 @default.
- W3098805361 creator A5091327770 @default.
- W3098805361 creator A5091592882 @default.
- W3098805361 date "2016-11-18" @default.
- W3098805361 modified "2023-10-17" @default.
- W3098805361 title "THE SPACE DENSITY OF LUMINOUS DUSTY STAR-FORMING GALAXIES AT<i>z</i>> 4: SCUBA-2 AND LABOCA IMAGING OF ULTRARED GALAXIES FROM<i>HERSCHEL</i>-ATLAS" @default.
- W3098805361 cites W1484400061 @default.
- W3098805361 cites W1570059738 @default.
- W3098805361 cites W1681063222 @default.
- W3098805361 cites W1821429365 @default.
- W3098805361 cites W1905466794 @default.
- W3098805361 cites W1917496003 @default.
- W3098805361 cites W1930424845 @default.
- W3098805361 cites W1969832966 @default.
- W3098805361 cites W1972016247 @default.
- W3098805361 cites W1975627161 @default.
- W3098805361 cites W1975977620 @default.
- W3098805361 cites W1994550968 @default.
- W3098805361 cites W1995047289 @default.
- W3098805361 cites W2004084407 @default.
- W3098805361 cites W2017100570 @default.
- W3098805361 cites W2017569741 @default.
- W3098805361 cites W2031076586 @default.
- W3098805361 cites W2043533977 @default.
- W3098805361 cites W2045977584 @default.
- W3098805361 cites W2047156688 @default.
- W3098805361 cites W2049565733 @default.
- W3098805361 cites W2054131667 @default.
- W3098805361 cites W2057589371 @default.
- W3098805361 cites W2058152646 @default.
- W3098805361 cites W2063814094 @default.
- W3098805361 cites W2074991347 @default.
- W3098805361 cites W2079304679 @default.
- W3098805361 cites W2079823208 @default.
- W3098805361 cites W2083468542 @default.
- W3098805361 cites W2094504621 @default.
- W3098805361 cites W2096624375 @default.
- W3098805361 cites W2109401568 @default.
- W3098805361 cites W2112633422 @default.
- W3098805361 cites W2117322039 @default.
- W3098805361 cites W2120875714 @default.
- W3098805361 cites W2126760679 @default.
- W3098805361 cites W2132759038 @default.
- W3098805361 cites W2133308199 @default.
- W3098805361 cites W2133581151 @default.
- W3098805361 cites W2134988917 @default.
- W3098805361 cites W2135536375 @default.
- W3098805361 cites W2135944207 @default.
- W3098805361 cites W2137454077 @default.
- W3098805361 cites W2138093180 @default.
- W3098805361 cites W2141444993 @default.
- W3098805361 cites W2150780877 @default.
- W3098805361 cites W2155870677 @default.
- W3098805361 cites W2160961312 @default.
- W3098805361 cites W2162511570 @default.
- W3098805361 cites W2165924595 @default.
- W3098805361 cites W2168495929 @default.
- W3098805361 cites W2168609373 @default.
- W3098805361 cites W2170568653 @default.
- W3098805361 cites W2236266652 @default.
- W3098805361 cites W2300756355 @default.
- W3098805361 cites W2340612067 @default.
- W3098805361 cites W2468936792 @default.
- W3098805361 cites W2952545856 @default.
- W3098805361 cites W2964210593 @default.
- W3098805361 cites W3099196797 @default.
- W3098805361 cites W3099326044 @default.
- W3098805361 cites W3099445393 @default.