FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1889105163> ?p ?o ?g. }

• W1889105163 endingPage "1184" @default.
• W1889105163 startingPage "1181" @default.
• W1889105163 abstract "Using evolutionary population synthesis, we present 13 refined absorption-line indices defined by the Lick Observatory Image Dissector Scanner (Lick/IDS) system for an extensive set of instantaneous-burst binary stellar populations (BSPs) at high resolution (similar to 0.3 angstrom), and 38 indices at intermediate resolution (3 angstrom). The ages of the populations are at an interval of 1 Gyr in the range 1-15 Gyr, and the metallicities are in the range 0.004-0.03. These indices are obtained by two methods: (i) using the empirical fitting functions (FFs method); (ii) measured directly from the synthetic spectra (DC method). Together with our previous paper, a data base of Lick/IDS spectral absorption-line indices for BSPs at high and intermediate resolutions is provided. This set of indices includes 21 indices of Worthey et al., four Balmer indices defined by Worthey & Ottaviani, and 13 indices with the new passband definitions of Trager et al. The full set of synthetic indices and the integrated pseudo-continuum are listed in the Appendices, which are only available online at http://www.blackwell-synergy.com/ or from our website (http://www.ast9.com/), or on request from the first author. Moreover, the full set of the integrated spectral energy distributions can be obtained from our website. We compare the synthetic Lick/IDS indices obtained by the FFs method and those by the DC method for BSPs with various metallicities, and find that the discrepancies are significant: Ca4455 (index 6), Fe4668 (8), Mg-b (13), Fe5709 (17), NaD (19), TiO1 (20) and TiO2 (21, except for Z = 0.02) in the W94 system, Ca4455(T) (6(T)), C(2)4668(T) (8(T)), NaDT (19(T)), TiO1T (20(T)) and TiO2T (21(T), except for Z = 0.02) in the T98 system obtained by the DC method are less (bluer) than the corresponding ones obtained by the FFs method for all metallicities. Ca4227 (index 3), Fe5782 (18), Ca4227(T) (3(T)) and Fe5782(T) (18(T)) are greater at Z = 0.03 and become bluer at Z = 0.004; the Fe5709(T) (17(T)) index is less at Z = 0.03 and becomes redder at Z = 0.004 than the corresponding ones obtained by the FFs method." @default.
• W1889105163 created "2016-06-24" @default.
• W1889105163 creator A5034116363 @default.
• W1889105163 creator A5039864059 @default.
• W1889105163 date "2006-06-16" @default.
• W1889105163 modified "2023-09-23" @default.
• W1889105163 title "A library of Lick Observatory Image Dissector Scanner indices for binary stellar populations" @default.
• W1889105163 cites W2017524870 @default.
• W1889105163 cites W2028207989 @default.
• W1889105163 cites W2080897707 @default.
• W1889105163 cites W2171413542 @default.
• W1889105163 cites W3099349192 @default.
• W1889105163 cites W3166554277 @default.
• W1889105163 doi "https://doi.org/10.1111/j.1365-2966.2006.10557.x" @default.
• W1889105163 hasPublicationYear "2006" @default.
• W1889105163 type Work @default.
• W1889105163 sameAs 1889105163 @default.
• W1889105163 citedByCount "7" @default.
• W1889105163 countsByYear W18891051632012 @default.
• W1889105163 countsByYear W18891051632013 @default.
• W1889105163 countsByYear W18891051632021 @default.
• W1889105163 crossrefType "journal-article" @default.
• W1889105163 hasAuthorship W1889105163A5034116363 @default.
• W1889105163 hasAuthorship W1889105163A5039864059 @default.
• W1889105163 hasConcept C120665830 @default.
• W1889105163 hasConcept C121332964 @default.
• W1889105163 hasConcept C1276947 @default.
• W1889105163 hasConcept C2779751349 @default.
• W1889105163 hasConcept C2779919027 @default.
• W1889105163 hasConcept C33923547 @default.
• W1889105163 hasConcept C44870925 @default.
• W1889105163 hasConcept C48372109 @default.
• W1889105163 hasConcept C94375191 @default.
• W1889105163 hasConceptScore W1889105163C120665830 @default.
• W1889105163 hasConceptScore W1889105163C121332964 @default.
• W1889105163 hasConceptScore W1889105163C1276947 @default.
• W1889105163 hasConceptScore W1889105163C2779751349 @default.
• W1889105163 hasConceptScore W1889105163C2779919027 @default.
• W1889105163 hasConceptScore W1889105163C33923547 @default.
• W1889105163 hasConceptScore W1889105163C44870925 @default.
• W1889105163 hasConceptScore W1889105163C48372109 @default.
• W1889105163 hasConceptScore W1889105163C94375191 @default.
• W1889105163 hasIssue "3" @default.
• W1889105163 hasLocation W18891051631 @default.
• W1889105163 hasOpenAccess W1889105163 @default.
• W1889105163 hasPrimaryLocation W18891051631 @default.
• W1889105163 hasRelatedWork W1989693711 @default.
• W1889105163 hasRelatedWork W1994702306 @default.
• W1889105163 hasRelatedWork W2010133960 @default.
• W1889105163 hasRelatedWork W2010201075 @default.
• W1889105163 hasRelatedWork W2029125027 @default.
• W1889105163 hasRelatedWork W2047375925 @default.
• W1889105163 hasRelatedWork W2069375389 @default.
• W1889105163 hasRelatedWork W2091176966 @default.
• W1889105163 hasRelatedWork W2147774829 @default.
• W1889105163 hasRelatedWork W3106428885 @default.
• W1889105163 hasVolume "370" @default.
• W1889105163 isParatext "false" @default.
• W1889105163 isRetracted "false" @default.
• W1889105163 magId "1889105163" @default.
• W1889105163 workType "article" @default.