Kepler and the Long Period Variables
High precision Kepler photometry is used to explore the details of AGB light curves. Since AGB variability has a typical time scale on order of a year we present methods for the removal of long term trends and quarterly changes in Kepler data. While undergoing long period variations of many magnitud...
| Main Authors: | , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2015-01-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/201510106032 |
| _version_ | 1819132593275142144 |
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| author | Hartig E. Cash J. Hinkle K. Lebzelter T. Mighell J. Walter D. K. |
| author_facet | Hartig E. Cash J. Hinkle K. Lebzelter T. Mighell J. Walter D. K. |
| author_sort | Hartig E. |
| collection | DOAJ |
| description | High precision Kepler photometry is used to explore the details of AGB light curves. Since AGB variability has a typical time scale on order of a year we present methods for the removal of long term trends and quarterly changes in Kepler data. While undergoing long period variations of many magnitudes, the light curves are shown to be smooth at the millimagnitude level over much shorter time intervals. No flares or other rapid events were detected down to the sub-day time scale. |
| first_indexed | 2024-12-22T09:33:52Z |
| format | Article |
| id | doaj.art-36bfc4ad17ad47f78d8cec2f6c5c4ade |
| institution | Directory Open Access Journal |
| issn | 2100-014X |
| language | English |
| last_indexed | 2024-12-22T09:33:52Z |
| publishDate | 2015-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| series | EPJ Web of Conferences |
| spelling | doaj.art-36bfc4ad17ad47f78d8cec2f6c5c4ade2022-12-21T18:30:52ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-011010603210.1051/epjconf/201510106032epjconf_sphr2014_06032Kepler and the Long Period VariablesHartig E.0Cash J.1Hinkle K.2Lebzelter T.3Mighell J.4Walter D. K.5University of Vienna, Department of AstrophysicsDepartment of Biological and Physical Sciences, South Carolina State UniversityNational Optical Astronomy ObservatoriesUniversity of Vienna, Department of AstrophysicsNational Optical Astronomy ObservatoriesDepartment of Biological and Physical Sciences, South Carolina State UniversityHigh precision Kepler photometry is used to explore the details of AGB light curves. Since AGB variability has a typical time scale on order of a year we present methods for the removal of long term trends and quarterly changes in Kepler data. While undergoing long period variations of many magnitudes, the light curves are shown to be smooth at the millimagnitude level over much shorter time intervals. No flares or other rapid events were detected down to the sub-day time scale.http://dx.doi.org/10.1051/epjconf/201510106032 |
| spellingShingle | Hartig E. Cash J. Hinkle K. Lebzelter T. Mighell J. Walter D. K. Kepler and the Long Period Variables EPJ Web of Conferences |
| title | Kepler and the Long Period Variables |
| title_full | Kepler and the Long Period Variables |
| title_fullStr | Kepler and the Long Period Variables |
| title_full_unstemmed | Kepler and the Long Period Variables |
| title_short | Kepler and the Long Period Variables |
| title_sort | kepler and the long period variables |
| url | http://dx.doi.org/10.1051/epjconf/201510106032 |
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