Matches in SemOpenAlex for { <https://semopenalex.org/work/W3104395689> ?p ?o ?g. }
- W3104395689 endingPage "2010" @default.
- W3104395689 startingPage "1998" @default.
- W3104395689 abstract "Fitting whole spectra at intermediate spectral resolution (R= 1000–3000), to derive physical properties of stellar populations, appears as an optimized alternative to methods based on spectrophotometric indices: it uses all the redundant information contained in the signal. This paper addresses the validation of the method and it investigates the quality of the population models together with the reliability of the fitting procedures. Our method compares observed optical spectra with models to derive the age, metallicity and line broadening due to the internal kinematics. It is insensitive to the shape of the continuum and the results are consistent with Lick indices but three times more precise. We are using two algorithms: steckmap, a non-parametric regularized program and nbursts a parametric non-linear minimization." @default.
- W3104395689 created "2020-11-23" @default.
- W3104395689 creator A5021142098 @default.
- W3104395689 creator A5034768562 @default.
- W3104395689 creator A5046499010 @default.
- W3104395689 creator A5047587237 @default.
- W3104395689 creator A5053832747 @default.
- W3104395689 date "2008-04-01" @default.
- W3104395689 modified "2023-10-18" @default.
- W3104395689 title "Spectroscopic ages and metallicities of stellar populations: validation of full spectrum fitting" @default.
- W3104395689 cites W1971196682 @default.
- W3104395689 cites W1974732677 @default.
- W3104395689 cites W1978850795 @default.
- W3104395689 cites W1982032918 @default.
- W3104395689 cites W1986771079 @default.
- W3104395689 cites W1993051956 @default.
- W3104395689 cites W1994574264 @default.
- W3104395689 cites W1994671833 @default.
- W3104395689 cites W1997384998 @default.
- W3104395689 cites W1998280804 @default.
- W3104395689 cites W2004783188 @default.
- W3104395689 cites W2020566995 @default.
- W3104395689 cites W2027924499 @default.
- W3104395689 cites W2028207989 @default.
- W3104395689 cites W2030216825 @default.
- W3104395689 cites W2062472109 @default.
- W3104395689 cites W2063232778 @default.
- W3104395689 cites W2066406099 @default.
- W3104395689 cites W2070543749 @default.
- W3104395689 cites W2088034685 @default.
- W3104395689 cites W2095777814 @default.
- W3104395689 cites W2096643625 @default.
- W3104395689 cites W2099955627 @default.
- W3104395689 cites W2105535379 @default.
- W3104395689 cites W2109521785 @default.
- W3104395689 cites W2110253451 @default.
- W3104395689 cites W2127401288 @default.
- W3104395689 cites W2132884113 @default.
- W3104395689 cites W2133712056 @default.
- W3104395689 cites W2134770831 @default.
- W3104395689 cites W2145398965 @default.
- W3104395689 cites W2151684988 @default.
- W3104395689 cites W2161928458 @default.
- W3104395689 cites W2163117531 @default.
- W3104395689 cites W2276444800 @default.
- W3104395689 cites W3099665156 @default.
- W3104395689 cites W3099811482 @default.
- W3104395689 cites W3099884674 @default.
- W3104395689 cites W3102716946 @default.
- W3104395689 cites W3103396469 @default.
- W3104395689 cites W3121651637 @default.
- W3104395689 cites W3166554277 @default.
- W3104395689 cites W4245623271 @default.
- W3104395689 cites W4248489183 @default.
- W3104395689 cites W4297889203 @default.
- W3104395689 cites W4301421064 @default.
- W3104395689 cites W4301944717 @default.
- W3104395689 doi "https://doi.org/10.1111/j.1365-2966.2008.12908.x" @default.
- W3104395689 hasPublicationYear "2008" @default.
- W3104395689 type Work @default.
- W3104395689 sameAs 3104395689 @default.
- W3104395689 citedByCount "149" @default.
- W3104395689 countsByYear W31043956892012 @default.
- W3104395689 countsByYear W31043956892013 @default.
- W3104395689 countsByYear W31043956892014 @default.
- W3104395689 countsByYear W31043956892015 @default.
- W3104395689 countsByYear W31043956892016 @default.
- W3104395689 countsByYear W31043956892017 @default.
- W3104395689 countsByYear W31043956892018 @default.
- W3104395689 countsByYear W31043956892019 @default.
- W3104395689 countsByYear W31043956892020 @default.
- W3104395689 countsByYear W31043956892021 @default.
- W3104395689 countsByYear W31043956892022 @default.
- W3104395689 countsByYear W31043956892023 @default.
- W3104395689 crossrefType "journal-article" @default.
- W3104395689 hasAuthorship W3104395689A5021142098 @default.
- W3104395689 hasAuthorship W3104395689A5034768562 @default.
- W3104395689 hasAuthorship W3104395689A5046499010 @default.
- W3104395689 hasAuthorship W3104395689A5047587237 @default.
- W3104395689 hasAuthorship W3104395689A5053832747 @default.
- W3104395689 hasBestOaLocation W31043956891 @default.
- W3104395689 hasConcept C105795698 @default.
- W3104395689 hasConcept C11413529 @default.
- W3104395689 hasConcept C117251300 @default.
- W3104395689 hasConcept C121332964 @default.
- W3104395689 hasConcept C121864883 @default.
- W3104395689 hasConcept C125857072 @default.
- W3104395689 hasConcept C1276947 @default.
- W3104395689 hasConcept C131432281 @default.
- W3104395689 hasConcept C144024400 @default.
- W3104395689 hasConcept C149923435 @default.
- W3104395689 hasConcept C150846664 @default.
- W3104395689 hasConcept C198352243 @default.
- W3104395689 hasConcept C24574437 @default.
- W3104395689 hasConcept C2524010 @default.
- W3104395689 hasConcept C2778623024 @default.
- W3104395689 hasConcept C2908647359 @default.
- W3104395689 hasConcept C33923547 @default.