Matches in SemOpenAlex for { <https://semopenalex.org/work/W3124371459> ?p ?o ?g. }
- W3124371459 endingPage "128" @default.
- W3124371459 startingPage "128" @default.
- W3124371459 abstract "We exploit the continuity equation approach and main-sequence star formation timescales to show that the observed high abundance of galaxies with stellar masses ≳ a few 1010 M⊙ at redshift z ≳ 4 implies the existence of a galaxy population featuring large star formation rates (SFRs) ψ ≳ 102 M⊙ yr−1 in heavily dust-obscured conditions. These galaxies constitute the high-redshift counterparts of the dusty star-forming population already surveyed for z ≲ 3 in the far-IR band by the Herschel Space Observatory. We work out specific predictions for the evolution of the corresponding stellar mass and SFR functions out to z ∼ 10, determining that the number density at z ≲ 8 for SFRs ψ ≳ 30 M⊙ yr−1 cannot be estimated relying on the UV luminosity function alone, even when standard corrections for dust extinction based on the UV slope are applied. We compute the number counts and redshift distributions (including galaxy-scale gravitational lensing) of this galaxy population, and show that current data from the AzTEC-LABOCA, SCUBA-2, and ALMA-SPT surveys are already addressing it. We demonstrate how an observational strategy based on color preselection in the far-IR or (sub-)millimeter band with Herschel and SCUBA-2, supplemented by photometric data from on-source observations with ALMA, can allow us to reconstruct the bright end of the SFR functions out to z ≲ 8. In parallel, such a challenging task can be managed by exploiting current UV surveys in combination with (sub-)millimeter observations by ALMA and NIKA2 and/or radio observations by SKA and its precursors." @default.
- W3124371459 created "2021-02-01" @default.
- W3124371459 creator A5017677240 @default.
- W3124371459 creator A5041560024 @default.
- W3124371459 creator A5042132634 @default.
- W3124371459 creator A5047200520 @default.
- W3124371459 creator A5051026292 @default.
- W3124371459 creator A5061666272 @default.
- W3124371459 date "2016-05-31" @default.
- W3124371459 modified "2023-10-18" @default.
- W3124371459 title "THE QUEST FOR DUSTY STAR-FORMING GALAXIES AT HIGH REDSHIFT<i>z</i>≳ 4" @default.
- W3124371459 cites W1492972489 @default.
- W3124371459 cites W1509944718 @default.
- W3124371459 cites W1582953240 @default.
- W3124371459 cites W1590758972 @default.
- W3124371459 cites W1603779598 @default.
- W3124371459 cites W1618397794 @default.
- W3124371459 cites W1848338669 @default.
- W3124371459 cites W1908085087 @default.
- W3124371459 cites W1912798299 @default.
- W3124371459 cites W1929287038 @default.
- W3124371459 cites W1948197607 @default.
- W3124371459 cites W1971002020 @default.
- W3124371459 cites W1973808059 @default.
- W3124371459 cites W1974288578 @default.
- W3124371459 cites W1975977620 @default.
- W3124371459 cites W1984849060 @default.
- W3124371459 cites W1986133984 @default.
- W3124371459 cites W1993384070 @default.
- W3124371459 cites W1994097808 @default.
- W3124371459 cites W1994550968 @default.
- W3124371459 cites W1997662069 @default.
- W3124371459 cites W2000030959 @default.
- W3124371459 cites W2000302520 @default.
- W3124371459 cites W2007442140 @default.
- W3124371459 cites W2008991538 @default.
- W3124371459 cites W2009886487 @default.
- W3124371459 cites W2013741966 @default.
- W3124371459 cites W2017047032 @default.
- W3124371459 cites W2018148195 @default.
- W3124371459 cites W2019562528 @default.
- W3124371459 cites W2025105301 @default.
- W3124371459 cites W2027113191 @default.
- W3124371459 cites W2027297109 @default.
- W3124371459 cites W2029466024 @default.
- W3124371459 cites W2029965202 @default.
- W3124371459 cites W2031076586 @default.
- W3124371459 cites W2034241894 @default.
- W3124371459 cites W2034353429 @default.
- W3124371459 cites W2036920580 @default.
- W3124371459 cites W2037526471 @default.
- W3124371459 cites W2039879975 @default.
- W3124371459 cites W2045491779 @default.
- W3124371459 cites W2045977584 @default.
- W3124371459 cites W2048316219 @default.
- W3124371459 cites W2052024199 @default.
- W3124371459 cites W2052923345 @default.
- W3124371459 cites W2053591448 @default.
- W3124371459 cites W2053644183 @default.
- W3124371459 cites W2054480927 @default.
- W3124371459 cites W2054857038 @default.
- W3124371459 cites W2063814094 @default.
- W3124371459 cites W2067649418 @default.
- W3124371459 cites W2068095952 @default.
- W3124371459 cites W2070696493 @default.
- W3124371459 cites W2072345977 @default.
- W3124371459 cites W2074037441 @default.
- W3124371459 cites W2074259895 @default.
- W3124371459 cites W2075105252 @default.
- W3124371459 cites W2086105458 @default.
- W3124371459 cites W2087459521 @default.
- W3124371459 cites W2088650185 @default.
- W3124371459 cites W2088821063 @default.
- W3124371459 cites W2090727515 @default.
- W3124371459 cites W2091010926 @default.
- W3124371459 cites W2091596771 @default.
- W3124371459 cites W2092504858 @default.
- W3124371459 cites W2094181926 @default.
- W3124371459 cites W2094871238 @default.
- W3124371459 cites W2096276600 @default.
- W3124371459 cites W2096624375 @default.
- W3124371459 cites W2103987722 @default.
- W3124371459 cites W2105929869 @default.
- W3124371459 cites W2107451664 @default.
- W3124371459 cites W2109774665 @default.
- W3124371459 cites W2111380403 @default.
- W3124371459 cites W2111600051 @default.
- W3124371459 cites W2112461408 @default.
- W3124371459 cites W2113686234 @default.
- W3124371459 cites W2114978259 @default.
- W3124371459 cites W2117637797 @default.
- W3124371459 cites W2121173473 @default.
- W3124371459 cites W2123267088 @default.
- W3124371459 cites W2123628940 @default.
- W3124371459 cites W2124602325 @default.
- W3124371459 cites W2124924585 @default.
- W3124371459 cites W2127888248 @default.
- W3124371459 cites W2129153205 @default.