FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3099390633> ?p ?o ?g. }

• W3099390633 endingPage "126" @default.
• W3099390633 startingPage "126" @default.
• W3099390633 abstract "It has been proposed that the mass-metallicity relation of galaxies exhibits a secondary dependence on star formation rate (SFR), and that the resulting M-Z-SFR relation may be redshift-invariant, i.e., fundamental. However, conflicting results on the character of the SFR dependence, and whether it exists, have been reported. To gain insight into the origins of the conflicting results, we (a) devise a non-parametric, astrophysically motivated analysis framework based on the offset from the star-forming (main) sequence at a given stellar mass (relative specific SFR), (b) apply this methodology and perform a comprehensive re-analysis of the local M-Z-SFR relation, based on SDSS, GALEX, and WISE data, and (c) study the impact of sample selection, and of using different metallicity and SFR indicators. We show that metallicity is anti-correlated with specific SFR regardless of the indicators used. We do not find that the relation is spurious due to correlations arising from biased metallicity measurements, or fiber aperture effects. We emphasize that the dependence is weak/absent for massive galaxies ($log M_*>10.5$), and that the overall scatter in the M-Z-SFR relation does not greatly decrease from the M-Z relation. We find that the dependence is stronger for the highest SSFR galaxies above the star-forming sequence. This two-mode behavior can be described with a broken linear fit in 12+log(O/H) vs. log (SFR$/M_*$), at a given $M_*$. Previous parameterizations used for comparative analysis with higher redshift samples that do not account for the more detailed behavior of the local M-Z-SFR relation may incorrectly lead to the conclusion that those samples follow a different relationship." @default.
• W3099390633 created "2020-11-23" @default.
• W3099390633 creator A5001016126 @default.
• W3099390633 creator A5027602092 @default.
• W3099390633 creator A5030391658 @default.
• W3099390633 creator A5053667167 @default.
• W3099390633 creator A5062524975 @default.
• W3099390633 creator A5065754893 @default.
• W3099390633 creator A5074138403 @default.
• W3099390633 creator A5075263706 @default.
• W3099390633 date "2014-12-08" @default.
• W3099390633 modified "2023-10-17" @default.
• W3099390633 title "A CRITICAL LOOK AT THE MASS-METALLICITY-STAR FORMATION RATE RELATION IN THE LOCAL UNIVERSE. I. AN IMPROVED ANALYSIS FRAMEWORK AND CONFOUNDING SYSTEMATICS" @default.
• W3099390633 cites W1598551420 @default.
• W3099390633 cites W1609394926 @default.
• W3099390633 cites W1671712505 @default.
• W3099390633 cites W1747250602 @default.
• W3099390633 cites W1855741887 @default.
• W3099390633 cites W1907943271 @default.
• W3099390633 cites W1911903648 @default.
• W3099390633 cites W1964280853 @default.
• W3099390633 cites W1964616701 @default.
• W3099390633 cites W1965970544 @default.
• W3099390633 cites W1966867730 @default.
• W3099390633 cites W1967876247 @default.
• W3099390633 cites W1968547533 @default.
• W3099390633 cites W1973758596 @default.
• W3099390633 cites W1976164719 @default.
• W3099390633 cites W1986426020 @default.
• W3099390633 cites W1992570077 @default.
• W3099390633 cites W1994671833 @default.
• W3099390633 cites W1996639384 @default.
• W3099390633 cites W1996738326 @default.
• W3099390633 cites W1997015919 @default.
• W3099390633 cites W1997662069 @default.
• W3099390633 cites W2000470824 @default.
• W3099390633 cites W2003635405 @default.
• W3099390633 cites W2008429960 @default.
• W3099390633 cites W2011654732 @default.
• W3099390633 cites W2012759655 @default.
• W3099390633 cites W2013575191 @default.
• W3099390633 cites W2026619221 @default.
• W3099390633 cites W2028626541 @default.
• W3099390633 cites W2030579627 @default.
• W3099390633 cites W2032949105 @default.
• W3099390633 cites W2034354443 @default.
• W3099390633 cites W2036491734 @default.
• W3099390633 cites W2045281485 @default.
• W3099390633 cites W2045308516 @default.
• W3099390633 cites W2045895958 @default.
• W3099390633 cites W2046457011 @default.
• W3099390633 cites W2049698250 @default.
• W3099390633 cites W2052937506 @default.
• W3099390633 cites W2056287285 @default.
• W3099390633 cites W2058889425 @default.
• W3099390633 cites W2063601622 @default.
• W3099390633 cites W2067857092 @default.
• W3099390633 cites W2069399805 @default.
• W3099390633 cites W2073262056 @default.
• W3099390633 cites W2074094455 @default.
• W3099390633 cites W2074976924 @default.
• W3099390633 cites W2077439896 @default.
• W3099390633 cites W2078833849 @default.
• W3099390633 cites W2089258422 @default.
• W3099390633 cites W2089947188 @default.
• W3099390633 cites W2093632493 @default.
• W3099390633 cites W2095644481 @default.
• W3099390633 cites W2096147217 @default.
• W3099390633 cites W2099650156 @default.
• W3099390633 cites W2107436274 @default.
• W3099390633 cites W2117199355 @default.
• W3099390633 cites W2121142967 @default.
• W3099390633 cites W2122893361 @default.
• W3099390633 cites W2123267088 @default.
• W3099390633 cites W2124181276 @default.
• W3099390633 cites W2126409956 @default.
• W3099390633 cites W2128384154 @default.
• W3099390633 cites W2141444467 @default.
• W3099390633 cites W2144334431 @default.
• W3099390633 cites W2145002594 @default.
• W3099390633 cites W2151062050 @default.
• W3099390633 cites W2163212281 @default.
• W3099390633 cites W2166365370 @default.
• W3099390633 cites W2166805045 @default.
• W3099390633 cites W2167262338 @default.
• W3099390633 cites W2167635287 @default.
• W3099390633 cites W2204815181 @default.
• W3099390633 cites W3098028737 @default.
• W3099390633 cites W3098813210 @default.
• W3099390633 cites W3098872520 @default.
• W3099390633 cites W3099149995 @default.
• W3099390633 cites W3099455476 @default.
• W3099390633 cites W3100172286 @default.
• W3099390633 cites W3100433659 @default.
• W3099390633 cites W3101362839 @default.
• W3099390633 cites W3101883929 @default.
• W3099390633 cites W3103139228 @default.
• W3099390633 cites W3103415621 @default.

• next