Matches in SemOpenAlex for { <https://semopenalex.org/work/W3099466648> ?p ?o ?g. }
- W3099466648 abstract "The RAdial Velocity Experiment (RAVE) is a spectroscopic survey of the Milky Way. We use the subsample of spectra with spectroscopically determined values of stellar parameters to determine the distances to these stars. The list currently contains 235,064 high quality spectra which show no peculiarities and belong to 210,872 different stars. The numbers will grow as the RAVE survey progresses. The public version of the catalog will be made available through the CDS services along with the ongoing RAVE public data releases. The distances are determined with a method based on the work by Breddels et al.~(2010). Here we assume that the star undergoes a standard stellar evolution and that its spectrum shows no peculiarities. The refinements include: the use of either of the three isochrone sets, a better account of the stellar ages and masses, use of more realistic errors of stellar parameter values, and application to a larger dataset. The derived distances of both dwarfs and giants match within ~21% to the astrometric distances of Hipparcos stars and to the distances of observed members of open and globular clusters. Multiple observations of a fraction of RAVE stars show that repeatability of the derived distances is even better, with half of the objects showing a distance scatter of simlt 11%. RAVE dwarfs are ~300 pc from the Sun, and giants are at distances of 1 to 2 kpc, and up to 10 kpc. This places the RAVE dataset between the more local Geneva-Copenhagen survey and the more distant and fainter SDSS sample. As such it is ideal to address some of the fundamental questions of Galactic structure and evolution in the pre-Gaia era. Individual applications are left to separate papers, here we show that the full 6-dimensional information on position and velocity is accurate enough to discuss the vertical structure and kinematic properties of the thin and thick disks." @default.
- W3099466648 created "2020-11-23" @default.
- W3099466648 creator A5006192532 @default.
- W3099466648 creator A5007394468 @default.
- W3099466648 creator A5007731573 @default.
- W3099466648 creator A5008041848 @default.
- W3099466648 creator A5010677439 @default.
- W3099466648 creator A5011784347 @default.
- W3099466648 creator A5012236841 @default.
- W3099466648 creator A5015365574 @default.
- W3099466648 creator A5028595054 @default.
- W3099466648 creator A5029582179 @default.
- W3099466648 creator A5037771086 @default.
- W3099466648 creator A5039501010 @default.
- W3099466648 creator A5042420253 @default.
- W3099466648 creator A5046542505 @default.
- W3099466648 creator A5047940369 @default.
- W3099466648 creator A5053675501 @default.
- W3099466648 creator A5060124457 @default.
- W3099466648 creator A5064352464 @default.
- W3099466648 creator A5070336889 @default.
- W3099466648 creator A5071789969 @default.
- W3099466648 creator A5073770015 @default.
- W3099466648 creator A5076154197 @default.
- W3099466648 creator A5078808074 @default.
- W3099466648 creator A5080448122 @default.
- W3099466648 creator A5084994654 @default.
- W3099466648 creator A5088453908 @default.
- W3099466648 date "2010-07-26" @default.
- W3099466648 modified "2023-10-05" @default.
- W3099466648 title "Distance determination for RAVE stars using stellar models II: Most likely values assuming a standard stellar evolution scenario" @default.
- W3099466648 cites W2097353541 @default.
- W3099466648 cites W3124077099 @default.
- W3099466648 hasPublicationYear "2010" @default.
- W3099466648 type Work @default.
- W3099466648 sameAs 3099466648 @default.
- W3099466648 citedByCount "0" @default.
- W3099466648 crossrefType "journal-article" @default.
- W3099466648 hasAuthorship W3099466648A5006192532 @default.
- W3099466648 hasAuthorship W3099466648A5007394468 @default.
- W3099466648 hasAuthorship W3099466648A5007731573 @default.
- W3099466648 hasAuthorship W3099466648A5008041848 @default.
- W3099466648 hasAuthorship W3099466648A5010677439 @default.
- W3099466648 hasAuthorship W3099466648A5011784347 @default.
- W3099466648 hasAuthorship W3099466648A5012236841 @default.
- W3099466648 hasAuthorship W3099466648A5015365574 @default.
- W3099466648 hasAuthorship W3099466648A5028595054 @default.
- W3099466648 hasAuthorship W3099466648A5029582179 @default.
- W3099466648 hasAuthorship W3099466648A5037771086 @default.
- W3099466648 hasAuthorship W3099466648A5039501010 @default.
- W3099466648 hasAuthorship W3099466648A5042420253 @default.
- W3099466648 hasAuthorship W3099466648A5046542505 @default.
- W3099466648 hasAuthorship W3099466648A5047940369 @default.
- W3099466648 hasAuthorship W3099466648A5053675501 @default.
- W3099466648 hasAuthorship W3099466648A5060124457 @default.
- W3099466648 hasAuthorship W3099466648A5064352464 @default.
- W3099466648 hasAuthorship W3099466648A5070336889 @default.
- W3099466648 hasAuthorship W3099466648A5071789969 @default.
- W3099466648 hasAuthorship W3099466648A5073770015 @default.
- W3099466648 hasAuthorship W3099466648A5076154197 @default.
- W3099466648 hasAuthorship W3099466648A5078808074 @default.
- W3099466648 hasAuthorship W3099466648A5080448122 @default.
- W3099466648 hasAuthorship W3099466648A5084994654 @default.
- W3099466648 hasAuthorship W3099466648A5088453908 @default.
- W3099466648 hasConcept C113461152 @default.
- W3099466648 hasConcept C121332964 @default.
- W3099466648 hasConcept C1276947 @default.
- W3099466648 hasConcept C133725777 @default.
- W3099466648 hasConcept C150846664 @default.
- W3099466648 hasConcept C176673079 @default.
- W3099466648 hasConcept C180690934 @default.
- W3099466648 hasConcept C44870925 @default.
- W3099466648 hasConcept C52348108 @default.
- W3099466648 hasConcept C555520305 @default.
- W3099466648 hasConceptScore W3099466648C113461152 @default.
- W3099466648 hasConceptScore W3099466648C121332964 @default.
- W3099466648 hasConceptScore W3099466648C1276947 @default.
- W3099466648 hasConceptScore W3099466648C133725777 @default.
- W3099466648 hasConceptScore W3099466648C150846664 @default.
- W3099466648 hasConceptScore W3099466648C176673079 @default.
- W3099466648 hasConceptScore W3099466648C180690934 @default.
- W3099466648 hasConceptScore W3099466648C44870925 @default.
- W3099466648 hasConceptScore W3099466648C52348108 @default.
- W3099466648 hasConceptScore W3099466648C555520305 @default.
- W3099466648 hasOpenAccess W3099466648 @default.
- W3099466648 hasRelatedWork W1797588316 @default.
- W3099466648 hasRelatedWork W2028406335 @default.
- W3099466648 hasRelatedWork W2134167138 @default.
- W3099466648 hasRelatedWork W2152624376 @default.
- W3099466648 hasRelatedWork W2154470714 @default.
- W3099466648 hasRelatedWork W2167758423 @default.
- W3099466648 hasRelatedWork W2172161529 @default.
- W3099466648 hasRelatedWork W2400983630 @default.
- W3099466648 hasRelatedWork W2417465022 @default.
- W3099466648 hasRelatedWork W2766689466 @default.
- W3099466648 hasRelatedWork W2805475758 @default.
- W3099466648 hasRelatedWork W2889765967 @default.
- W3099466648 hasRelatedWork W2890196524 @default.
- W3099466648 hasRelatedWork W2960314319 @default.
- W3099466648 hasRelatedWork W2979492295 @default.