FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100433659> ?p ?o ?g. }

• W3100433659 abstract "We derive the mass-metallicity relation of star-forming galaxies up to $zsim0.9$, using data from the VIMOS VLT Deep Survey. Automatic measurement of emission-line fluxes and equivalent widths have been performed on the full spectroscopic sample. This sample is divided into two sub-samples depending on the apparent magnitude selection: wide ($I_{mathrm{AB}}<22.5$) and deep $I_{mathrm{AB}}<24$). These two samples span two different ranges of stellar masses. Emission-line galaxies have been separated into star-forming galaxies and active galactic nuclei using emission line ratios. For the star-forming galaxies the emission line ratios have also been used to estimate gas-phase oxygen abundance, using empirical calibrations renormalized in order to give consistent results at low and high redshifts. The stellar masses have been estimated by fitting the whole spectral energy distributions with a set of stellar population synthesis models. We assume at first order that the shape of the mass-metallicity relation remains constant with redshift. Then we find a stronger metallicity evolution in the wide sample as compared to the deep sample. We thus conclude that the mass-metallicity relation is flatter at higher redshift. The observed flattening of the mass-metallicity relation at high redshift is analyzed as an evidence in favor of the open-closed model." @default.
• W3100433659 created "2020-11-23" @default.
• W3100433659 creator A5001016126 @default.
• W3100433659 creator A5003060074 @default.
• W3100433659 creator A5006069743 @default.
• W3100433659 creator A5009404806 @default.
• W3100433659 creator A5015975135 @default.
• W3100433659 creator A5019158392 @default.
• W3100433659 creator A5021267951 @default.
• W3100433659 creator A5022137696 @default.
• W3100433659 creator A5022894838 @default.
• W3100433659 creator A5023314136 @default.
• W3100433659 creator A5023774207 @default.
• W3100433659 creator A5023869216 @default.
• W3100433659 creator A5025639742 @default.
• W3100433659 creator A5028548201 @default.
• W3100433659 creator A5029867699 @default.
• W3100433659 creator A5030920057 @default.
• W3100433659 creator A5031242872 @default.
• W3100433659 creator A5031917607 @default.
• W3100433659 creator A5032965755 @default.
• W3100433659 creator A5032993665 @default.
• W3100433659 creator A5033864066 @default.
• W3100433659 creator A5035438463 @default.
• W3100433659 creator A5035540139 @default.
• W3100433659 creator A5037658542 @default.
• W3100433659 creator A5041408764 @default.
• W3100433659 creator A5047214802 @default.
• W3100433659 creator A5051323119 @default.
• W3100433659 creator A5052031270 @default.
• W3100433659 creator A5055948382 @default.
• W3100433659 creator A5056456679 @default.
• W3100433659 creator A5060311084 @default.
• W3100433659 creator A5061935397 @default.
• W3100433659 creator A5062382923 @default.
• W3100433659 creator A5063341829 @default.
• W3100433659 creator A5068797292 @default.
• W3100433659 creator A5069101046 @default.
• W3100433659 creator A5075023487 @default.
• W3100433659 creator A5075132871 @default.
• W3100433659 creator A5081204604 @default.
• W3100433659 creator A5081479547 @default.
• W3100433659 creator A5081908574 @default.
• W3100433659 creator A5085221278 @default.
• W3100433659 creator A5088192303 @default.
• W3100433659 creator A5088219275 @default.
• W3100433659 creator A5090420192 @default.
• W3100433659 creator A5090478962 @default.
• W3100433659 date "2009-02-21" @default.
• W3100433659 modified "2023-10-18" @default.
• W3100433659 title "Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. I. The evolution of the mass-metallicity relation up to z~0.9" @default.
• W3100433659 doi "https://doi.org/10.1051/0004-6361:200810397" @default.
• W3100433659 hasPublicationYear "2009" @default.
• W3100433659 type Work @default.
• W3100433659 sameAs 3100433659 @default.
• W3100433659 citedByCount "81" @default.
• W3100433659 countsByYear W31004336592012 @default.
• W3100433659 countsByYear W31004336592013 @default.
• W3100433659 countsByYear W31004336592014 @default.
• W3100433659 countsByYear W31004336592015 @default.
• W3100433659 countsByYear W31004336592016 @default.
• W3100433659 countsByYear W31004336592017 @default.
• W3100433659 countsByYear W31004336592018 @default.
• W3100433659 countsByYear W31004336592019 @default.
• W3100433659 countsByYear W31004336592020 @default.
• W3100433659 countsByYear W31004336592021 @default.
• W3100433659 countsByYear W31004336592022 @default.
• W3100433659 countsByYear W31004336592023 @default.
• W3100433659 crossrefType "journal-article" @default.
• W3100433659 hasAuthorship W3100433659A5001016126 @default.
• W3100433659 hasAuthorship W3100433659A5003060074 @default.
• W3100433659 hasAuthorship W3100433659A5006069743 @default.
• W3100433659 hasAuthorship W3100433659A5009404806 @default.
• W3100433659 hasAuthorship W3100433659A5015975135 @default.
• W3100433659 hasAuthorship W3100433659A5019158392 @default.
• W3100433659 hasAuthorship W3100433659A5021267951 @default.
• W3100433659 hasAuthorship W3100433659A5022137696 @default.
• W3100433659 hasAuthorship W3100433659A5022894838 @default.
• W3100433659 hasAuthorship W3100433659A5023314136 @default.
• W3100433659 hasAuthorship W3100433659A5023774207 @default.
• W3100433659 hasAuthorship W3100433659A5023869216 @default.
• W3100433659 hasAuthorship W3100433659A5025639742 @default.
• W3100433659 hasAuthorship W3100433659A5028548201 @default.
• W3100433659 hasAuthorship W3100433659A5029867699 @default.
• W3100433659 hasAuthorship W3100433659A5030920057 @default.
• W3100433659 hasAuthorship W3100433659A5031242872 @default.
• W3100433659 hasAuthorship W3100433659A5031917607 @default.
• W3100433659 hasAuthorship W3100433659A5032965755 @default.
• W3100433659 hasAuthorship W3100433659A5032993665 @default.
• W3100433659 hasAuthorship W3100433659A5033864066 @default.
• W3100433659 hasAuthorship W3100433659A5035438463 @default.
• W3100433659 hasAuthorship W3100433659A5035540139 @default.
• W3100433659 hasAuthorship W3100433659A5037658542 @default.
• W3100433659 hasAuthorship W3100433659A5041408764 @default.
• W3100433659 hasAuthorship W3100433659A5047214802 @default.
• W3100433659 hasAuthorship W3100433659A5051323119 @default.
• W3100433659 hasAuthorship W3100433659A5052031270 @default.
• W3100433659 hasAuthorship W3100433659A5055948382 @default.
• W3100433659 hasAuthorship W3100433659A5056456679 @default.
• W3100433659 hasAuthorship W3100433659A5060311084 @default.

• next