FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3005407798> ?p ?o ?g. }

• W3005407798 abstract "We performed a theoretical analysis on the relevance of the small frequency separation $delta nu$ in determining stellar ages, masses, and radii. We adopted the SCEPtER pipeline for low-mass stars, [0.7, 1.05] Msun. Synthetic stars were generated and reconstructed assuming different relative precision in $delta nu$ (5% and 2%). The quantification of the systematic errors arising from a mismatch between synthetic stars and the recovery grid was also performed. The biases were negligible. The statistical error in age estimates was strongly dependent on the stellar evolutionary phase. It is at its maximum at ZAMS and decreases to about 11% and 6% ($delta nu$ at 5% and 2% level) when stars reach the 30% of their evolutionary MS lifetime, then vanishes in the last 20% of the MS. For mass and radius estimates we detected nearly identical behavior for an observational uncertainty of 5%. No benefit was detected for mass and radius determinations from a reduction $delta nu$ precision to 2%. The impact on the age of the initial helium abundance resulted in negligible results. On the other hand greater bias (2% and 1%) in mass and radius estimates were detected whenever $delta nu$ is in the observational pool. This result, together with the presence of further unexplored uncertainty sources, suggest that precision in the derived stellar quantities below these thresholds may possibly be overoptimistic. [...] Finally, we compared the estimates by the SCEPtER pipeline for 13 Kepler asteroseismic LEGACY sample stars with those given by six different pipelines. Overall, on the LEGACY sample data, we obtained a multi-pipeline precision of about 4.4%, 1.7%, and 11% on the estimated masses, radii, and ages, respectively." @default.
• W3005407798 created "2020-02-14" @default.
• W3005407798 creator A5013158855 @default.
• W3005407798 creator A5051901917 @default.
• W3005407798 creator A5054137091 @default.
• W3005407798 creator A5076825008 @default.
• W3005407798 date "2020-02-05" @default.
• W3005407798 modified "2023-09-27" @default.
• W3005407798 title "Relevance of the small frequency separation for asteroseismic stellar age, mass, and radius. A statistical investigation for main-sequence low-mass stars" @default.
• W3005407798 cites W1513591705 @default.
• W3005407798 cites W1654493013 @default.
• W3005407798 cites W1827099979 @default.
• W3005407798 cites W1933422323 @default.
• W3005407798 cites W1973500133 @default.
• W3005407798 cites W1986099565 @default.
• W3005407798 cites W1995519722 @default.
• W3005407798 cites W1998365924 @default.
• W3005407798 cites W2001471478 @default.
• W3005407798 cites W2006124034 @default.
• W3005407798 cites W2010885363 @default.
• W3005407798 cites W2020288645 @default.
• W3005407798 cites W2038961364 @default.
• W3005407798 cites W2048141122 @default.
• W3005407798 cites W2048905273 @default.
• W3005407798 cites W2061413477 @default.
• W3005407798 cites W2066738030 @default.
• W3005407798 cites W2080837761 @default.
• W3005407798 cites W2081142176 @default.
• W3005407798 cites W2082378688 @default.
• W3005407798 cites W2101075118 @default.
• W3005407798 cites W2105982231 @default.
• W3005407798 cites W2117029129 @default.
• W3005407798 cites W2119095722 @default.
• W3005407798 cites W2120415720 @default.
• W3005407798 cites W2124574813 @default.
• W3005407798 cites W2144214856 @default.
• W3005407798 cites W2147162230 @default.
• W3005407798 cites W2164080525 @default.
• W3005407798 cites W2204429661 @default.
• W3005407798 cites W2558422827 @default.
• W3005407798 cites W2562429066 @default.
• W3005407798 cites W2613458683 @default.
• W3005407798 cites W2773015712 @default.
• W3005407798 cites W2784746773 @default.
• W3005407798 cites W2797933484 @default.
• W3005407798 cites W2888086463 @default.
• W3005407798 cites W2899497983 @default.
• W3005407798 cites W2909449901 @default.
• W3005407798 cites W2949754020 @default.
• W3005407798 cites W3098019590 @default.
• W3005407798 cites W3099252578 @default.
• W3005407798 cites W3100304147 @default.
• W3005407798 cites W3101023157 @default.
• W3005407798 cites W3101382562 @default.
• W3005407798 cites W3101404695 @default.
• W3005407798 cites W3102678455 @default.
• W3005407798 cites W3103190686 @default.
• W3005407798 cites W3103639866 @default.
• W3005407798 cites W3104594662 @default.
• W3005407798 cites W3121888922 @default.
• W3005407798 cites W3122215177 @default.
• W3005407798 hasPublicationYear "2020" @default.
• W3005407798 type Work @default.
• W3005407798 sameAs 3005407798 @default.
• W3005407798 citedByCount "0" @default.
• W3005407798 crossrefType "journal-article" @default.
• W3005407798 hasAuthorship W3005407798A5013158855 @default.
• W3005407798 hasAuthorship W3005407798A5051901917 @default.
• W3005407798 hasAuthorship W3005407798A5054137091 @default.
• W3005407798 hasAuthorship W3005407798A5076825008 @default.
• W3005407798 hasBestOaLocation W30054077981 @default.
• W3005407798 hasConcept C110472602 @default.
• W3005407798 hasConcept C121332964 @default.
• W3005407798 hasConcept C125857072 @default.
• W3005407798 hasConcept C1276947 @default.
• W3005407798 hasConcept C150846664 @default.
• W3005407798 hasConcept C168589115 @default.
• W3005407798 hasConcept C178635117 @default.
• W3005407798 hasConcept C38652104 @default.
• W3005407798 hasConcept C41008148 @default.
• W3005407798 hasConcept C44870925 @default.
• W3005407798 hasConceptScore W3005407798C110472602 @default.
• W3005407798 hasConceptScore W3005407798C121332964 @default.
• W3005407798 hasConceptScore W3005407798C125857072 @default.
• W3005407798 hasConceptScore W3005407798C1276947 @default.
• W3005407798 hasConceptScore W3005407798C150846664 @default.
• W3005407798 hasConceptScore W3005407798C168589115 @default.
• W3005407798 hasConceptScore W3005407798C178635117 @default.
• W3005407798 hasConceptScore W3005407798C38652104 @default.
• W3005407798 hasConceptScore W3005407798C41008148 @default.
• W3005407798 hasConceptScore W3005407798C44870925 @default.
• W3005407798 hasLocation W30054077981 @default.
• W3005407798 hasLocation W30054077982 @default.
• W3005407798 hasOpenAccess W3005407798 @default.
• W3005407798 hasPrimaryLocation W30054077981 @default.
• W3005407798 hasRelatedWork W1827099979 @default.
• W3005407798 hasRelatedWork W2107643210 @default.
• W3005407798 hasRelatedWork W2115544639 @default.
• W3005407798 hasRelatedWork W2151861814 @default.
• W3005407798 hasRelatedWork W2164080525 @default.

• next