FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3122192693> ?p ?o ?g. }

• W3122192693 endingPage "A9" @default.
• W3122192693 startingPage "A9" @default.
• W3122192693 abstract "We investigate the effect of different star formation histories (SFHs) on the relation between stellar mass (M∗) and star formation rate (SFR) using a sample of galaxies with reliable spectroscopic redshift zspec> 2 drawn from the VIMOS Ultra-Deep Survey (VUDS). We produce an extensive database of dusty model galaxies, calculated starting from a new library of single stellar population (SSPs) models, weighted by a set of 28 different star formation histories based on the Schmidt function, and characterized by different ratios of the gas infall timescale τinfall to the star formation efficiency ν. Dust extinction and re-emission were treated by means of the radiative transfer calculation. The spectral energy distribution (SED) fitting technique was performed by using GOSSIP+, a tool able to combine both photometric and spectroscopic information to extract the best value of the physical quantities of interest, and to consider the intergalactic medium (IGM) attenuation as a free parameter. We find that the main contribution to the scatter observed in the SFR-M∗ plane is the possibility of choosing between different families of SFHs in the SED fitting procedure, while the redshift range plays a minor role. The majority of the galaxies, at all cosmic times, are best fit by models with SFHs characterized by a high τinfall/ν ratio. We discuss the reliability of a low percentage of dusty and highly star-forming galaxies in the context of their detection in the far infrared (FIR)." @default.
• W3122192693 created "2021-02-01" @default.
• W3122192693 creator A5001219575 @default.
• W3122192693 creator A5004163126 @default.
• W3122192693 creator A5004924198 @default.
• W3122192693 creator A5009392191 @default.
• W3122192693 creator A5019841800 @default.
• W3122192693 creator A5019896377 @default.
• W3122192693 creator A5020384219 @default.
• W3122192693 creator A5022137696 @default.
• W3122192693 creator A5022894838 @default.
• W3122192693 creator A5026007485 @default.
• W3122192693 creator A5026264699 @default.
• W3122192693 creator A5028548201 @default.
• W3122192693 creator A5029041235 @default.
• W3122192693 creator A5029531883 @default.
• W3122192693 creator A5029867699 @default.
• W3122192693 creator A5031917607 @default.
• W3122192693 creator A5035540139 @default.
• W3122192693 creator A5039049327 @default.
• W3122192693 creator A5039140400 @default.
• W3122192693 creator A5041079860 @default.
• W3122192693 creator A5041408764 @default.
• W3122192693 creator A5042004608 @default.
• W3122192693 creator A5043083140 @default.
• W3122192693 creator A5044536023 @default.
• W3122192693 creator A5048538677 @default.
• W3122192693 creator A5051323119 @default.
• W3122192693 creator A5051423042 @default.
• W3122192693 creator A5052031270 @default.
• W3122192693 creator A5053667167 @default.
• W3122192693 creator A5055948382 @default.
• W3122192693 creator A5058519861 @default.
• W3122192693 creator A5062010375 @default.
• W3122192693 creator A5067616980 @default.
• W3122192693 creator A5069101046 @default.
• W3122192693 creator A5072964779 @default.
• W3122192693 creator A5073097053 @default.
• W3122192693 creator A5075217338 @default.
• W3122192693 creator A5075527069 @default.
• W3122192693 creator A5080370301 @default.
• W3122192693 creator A5081052936 @default.
• W3122192693 creator A5081204604 @default.
• W3122192693 creator A5085221278 @default.
• W3122192693 creator A5086583377 @default.
• W3122192693 creator A5087241593 @default.
• W3122192693 creator A5089688228 @default.
• W3122192693 creator A5089867752 @default.
• W3122192693 creator A5091049430 @default.
• W3122192693 date "2016-08-29" @default.
• W3122192693 modified "2023-10-18" @default.
• W3122192693 title "Effect of the star formation histories on the<i>SFR</i>-<i>M</i>_∗relation at<i>z</i>≥ 2" @default.
• W3122192693 cites W1567460774 @default.
• W3122192693 cites W1602680202 @default.
• W3122192693 cites W1622230873 @default.
• W3122192693 cites W1833860403 @default.
• W3122192693 cites W1842880767 @default.
• W3122192693 cites W1964344398 @default.
• W3122192693 cites W1968131817 @default.
• W3122192693 cites W1968635501 @default.
• W3122192693 cites W1970196846 @default.
• W3122192693 cites W1970333333 @default.
• W3122192693 cites W1974174849 @default.
• W3122192693 cites W1983583637 @default.
• W3122192693 cites W1984615557 @default.
• W3122192693 cites W1985370957 @default.
• W3122192693 cites W1985952407 @default.
• W3122192693 cites W1993283828 @default.
• W3122192693 cites W1994671833 @default.
• W3122192693 cites W1997662069 @default.
• W3122192693 cites W2018539983 @default.
• W3122192693 cites W2020863669 @default.
• W3122192693 cites W2025913857 @default.
• W3122192693 cites W2029483560 @default.
• W3122192693 cites W2034241894 @default.
• W3122192693 cites W2034723625 @default.
• W3122192693 cites W2037970068 @default.
• W3122192693 cites W2048167631 @default.
• W3122192693 cites W2048414711 @default.
• W3122192693 cites W2049642912 @default.
• W3122192693 cites W2053265856 @default.
• W3122192693 cites W2077017611 @default.
• W3122192693 cites W2077410856 @default.
• W3122192693 cites W2081173787 @default.
• W3122192693 cites W2081942037 @default.
• W3122192693 cites W2090698037 @default.
• W3122192693 cites W2094560547 @default.
• W3122192693 cites W2095855161 @default.
• W3122192693 cites W2096276600 @default.
• W3122192693 cites W2100288398 @default.
• W3122192693 cites W2104138988 @default.
• W3122192693 cites W2114951275 @default.
• W3122192693 cites W2114978259 @default.
• W3122192693 cites W2116466430 @default.
• W3122192693 cites W2125977823 @default.
• W3122192693 cites W2126973721 @default.
• W3122192693 cites W2128904482 @default.
• W3122192693 cites W2148140550 @default.

• next