Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100019216> ?p ?o ?g. }
- W3100019216 endingPage "9" @default.
- W3100019216 startingPage "9" @default.
- W3100019216 abstract "We use the James Clerk Maxwell Telescope's SCUBA-2 camera to image a 400 arcmin2 area surrounding the GOODS-N field. The 850 μm rms noise ranges from a value of 0.49 mJy in the central region to 3.5 mJy at the outside edge. From these data, we construct an 850 μm source catalog to 2 mJy containing 49 sources detected above the 4σ level. We use an ultradeep (11.5 μJy at 5σ) 1.4 GHz image obtained with the Karl G. Jansky Very Large Array together with observations made with the Submillimeter Array to identify counterparts to the submillimeter galaxies. For most cases of multiple radio counterparts, we can identify the correct counterpart from new and existing Submillimeter Array data. We have spectroscopic redshifts for 62% of the radio sources in the 9' radius highest sensitivity region (556/894) and 67% of the radio sources in the GOODS-N region (367/543). We supplement these with a modest number of additional photometric redshifts in the GOODS-N region (30). We measure millimetric redshifts from the radio to submillimeter flux ratios for the unidentified submillimeter sample, assuming an Arp 220 spectral energy distribution. We find a radio-flux-dependent K − z relation for the radio sources, which we use to estimate redshifts for the remaining radio sources. We determine the star formation rates (SFRs) of the submillimeter sources based on their radio powers and their submillimeter fluxes and find that they agree well. The radio data are deep enough to detect star-forming galaxies with SFRs >2000 M☉ yr−1 to z ∼ 6. We find galaxies with SFRs up to ∼6000 M☉ yr−1 over the redshift range z = 1.5–6, but we see evidence for a turn-down in the SFR distribution function above 2000 M☉ yr−1." @default.
- W3100019216 created "2020-11-23" @default.
- W3100019216 creator A5011211151 @default.
- W3100019216 creator A5018536426 @default.
- W3100019216 creator A5031551491 @default.
- W3100019216 creator A5035445329 @default.
- W3100019216 creator A5051114623 @default.
- W3100019216 creator A5056348168 @default.
- W3100019216 creator A5077389758 @default.
- W3100019216 creator A5078199447 @default.
- W3100019216 creator A5086861709 @default.
- W3100019216 date "2014-02-26" @default.
- W3100019216 modified "2023-10-16" @default.
- W3100019216 title "IS THERE A MAXIMUM STAR FORMATION RATE IN HIGH-REDSHIFT GALAXIES?, , ," @default.
- W3100019216 cites W1498122459 @default.
- W3100019216 cites W1598902974 @default.
- W3100019216 cites W1634409775 @default.
- W3100019216 cites W1681063222 @default.
- W3100019216 cites W1748091613 @default.
- W3100019216 cites W1841113251 @default.
- W3100019216 cites W1851451509 @default.
- W3100019216 cites W1869747873 @default.
- W3100019216 cites W1880006316 @default.
- W3100019216 cites W1963915931 @default.
- W3100019216 cites W1965700990 @default.
- W3100019216 cites W1968809627 @default.
- W3100019216 cites W1970058472 @default.
- W3100019216 cites W1970315890 @default.
- W3100019216 cites W1973771337 @default.
- W3100019216 cites W1974305663 @default.
- W3100019216 cites W1974668797 @default.
- W3100019216 cites W1975478564 @default.
- W3100019216 cites W1980817659 @default.
- W3100019216 cites W1987400244 @default.
- W3100019216 cites W1994033192 @default.
- W3100019216 cites W1994124960 @default.
- W3100019216 cites W1996755716 @default.
- W3100019216 cites W1996990154 @default.
- W3100019216 cites W1997662069 @default.
- W3100019216 cites W1999046479 @default.
- W3100019216 cites W2005332378 @default.
- W3100019216 cites W2006676156 @default.
- W3100019216 cites W2008991538 @default.
- W3100019216 cites W2014203224 @default.
- W3100019216 cites W2015295900 @default.
- W3100019216 cites W2017450908 @default.
- W3100019216 cites W2017569741 @default.
- W3100019216 cites W2019866699 @default.
- W3100019216 cites W2020701654 @default.
- W3100019216 cites W2024028682 @default.
- W3100019216 cites W2025912137 @default.
- W3100019216 cites W2025969090 @default.
- W3100019216 cites W2028416059 @default.
- W3100019216 cites W2029965202 @default.
- W3100019216 cites W2031638105 @default.
- W3100019216 cites W2033021957 @default.
- W3100019216 cites W2033327477 @default.
- W3100019216 cites W2034892354 @default.
- W3100019216 cites W2043533977 @default.
- W3100019216 cites W2044093857 @default.
- W3100019216 cites W2044460462 @default.
- W3100019216 cites W2047758030 @default.
- W3100019216 cites W2048997571 @default.
- W3100019216 cites W2049565733 @default.
- W3100019216 cites W2049698250 @default.
- W3100019216 cites W2055548073 @default.
- W3100019216 cites W2060572005 @default.
- W3100019216 cites W2066800938 @default.
- W3100019216 cites W2069804077 @default.
- W3100019216 cites W2069896074 @default.
- W3100019216 cites W2070677059 @default.
- W3100019216 cites W2070952256 @default.
- W3100019216 cites W2073285288 @default.
- W3100019216 cites W2074037441 @default.
- W3100019216 cites W2074320758 @default.
- W3100019216 cites W2074976924 @default.
- W3100019216 cites W2078697049 @default.
- W3100019216 cites W2080739141 @default.
- W3100019216 cites W2088650185 @default.
- W3100019216 cites W2090561782 @default.
- W3100019216 cites W2094181926 @default.
- W3100019216 cites W2096559587 @default.
- W3100019216 cites W2104143670 @default.
- W3100019216 cites W2106414865 @default.
- W3100019216 cites W2109401568 @default.
- W3100019216 cites W2110294314 @default.
- W3100019216 cites W2116053549 @default.
- W3100019216 cites W2116466430 @default.
- W3100019216 cites W2122193056 @default.
- W3100019216 cites W2125279088 @default.
- W3100019216 cites W2126287728 @default.
- W3100019216 cites W2129760210 @default.
- W3100019216 cites W2131796255 @default.
- W3100019216 cites W2132759038 @default.
- W3100019216 cites W2133072968 @default.
- W3100019216 cites W2139681095 @default.
- W3100019216 cites W2151920714 @default.
- W3100019216 cites W2152912297 @default.