A fitting LEGACY – modelling Kepler's best stars
The LEGACY sample represents the best solar-like stars observed in the Kepler mission[5, 8]. The 66 stars in the sample are all on the main sequence or only slightly more evolved. They each have more than one year's observation data in short cadence, allowing for precise extraction of individua...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2017-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | https://doi.org/10.1051/epjconf/201716003010 |
| _version_ | 1819134004275707904 |
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| author | Aarslev Magnus J. Christensen-Dalsgaard Jørgen Lund Mikkel N. Aguirre Victor Silva Gough Douglas |
| author_facet | Aarslev Magnus J. Christensen-Dalsgaard Jørgen Lund Mikkel N. Aguirre Victor Silva Gough Douglas |
| author_sort | Aarslev Magnus J. |
| collection | DOAJ |
| description | The LEGACY sample represents the best solar-like stars observed in the Kepler mission[5, 8]. The 66 stars in the sample are all on the main sequence or only slightly more evolved. They each have more than one year's observation data in short cadence, allowing for precise extraction of individual frequencies. Here we present model fits using a modified ASTFIT procedure employing two different near-surface-effect corrections, one by Christensen-Dalsgaard[4] and a newer correction proposed by Ball & Gizon[1]. We then compare the results obtained using the different corrections. We find that using the latter correction yields lower masses and significantly lower χ2 values for a large part of the sample. |
| first_indexed | 2024-12-22T09:56:17Z |
| format | Article |
| id | doaj.art-5bc18e48b5c3485fa1b14c032e985a6e |
| institution | Directory Open Access Journal |
| issn | 2100-014X |
| language | English |
| last_indexed | 2024-12-22T09:56:17Z |
| publishDate | 2017-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| series | EPJ Web of Conferences |
| spelling | doaj.art-5bc18e48b5c3485fa1b14c032e985a6e2022-12-21T18:30:15ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011600301010.1051/epjconf/201716003010epjconf_azores2017_03010A fitting LEGACY – modelling Kepler's best starsAarslev Magnus J.Christensen-Dalsgaard JørgenLund Mikkel N.Aguirre Victor SilvaGough DouglasThe LEGACY sample represents the best solar-like stars observed in the Kepler mission[5, 8]. The 66 stars in the sample are all on the main sequence or only slightly more evolved. They each have more than one year's observation data in short cadence, allowing for precise extraction of individual frequencies. Here we present model fits using a modified ASTFIT procedure employing two different near-surface-effect corrections, one by Christensen-Dalsgaard[4] and a newer correction proposed by Ball & Gizon[1]. We then compare the results obtained using the different corrections. We find that using the latter correction yields lower masses and significantly lower χ2 values for a large part of the sample.https://doi.org/10.1051/epjconf/201716003010 |
| spellingShingle | Aarslev Magnus J. Christensen-Dalsgaard Jørgen Lund Mikkel N. Aguirre Victor Silva Gough Douglas A fitting LEGACY – modelling Kepler's best stars EPJ Web of Conferences |
| title | A fitting LEGACY – modelling Kepler's best stars |
| title_full | A fitting LEGACY – modelling Kepler's best stars |
| title_fullStr | A fitting LEGACY – modelling Kepler's best stars |
| title_full_unstemmed | A fitting LEGACY – modelling Kepler's best stars |
| title_short | A fitting LEGACY – modelling Kepler's best stars |
| title_sort | fitting legacy modelling kepler s best stars |
| url | https://doi.org/10.1051/epjconf/201716003010 |
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