Abstract
The advent of space-based telescopes in the last decade such as MOST, CoRoT and Kepler, has become known as the Space Photometry Revolution. The KeplerSpace Telescope provided high photometric precision, a high duty cycle and data spanning four years for approximately 200 000 stars. In this chapter, a review of the KeplerSpace Telescope is provided including relevant details of using Keplerdata for asteroseismology. Also, the processing of all Keplerobservations of A and F stars is discussed, which formed the data set to find all the delta Sct stars studied in this monograph.
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Notes
- 1.
This was the title of the CoRoT-3/KASC7 conference held in 2014: http://corot3-kasc7.sciencesconf.org. The conference proceedings for a poster by Bowman and Kurtz (2015) were published in the European Physical Journal Web of Conferences (EPJWC) from this conference.
- 2.
An up-to-date catalogue is available at: http://exoplanetarchive.ipac.caltech.edu.
- 3.
An up-to-date catalogue is available at: http://keplerebs.villanova.edu.
- 4.
KASOC website: http://www.kasoc.phys.au.dk.
- 5.
MAST website: http://archive.stsci.edu/kepler/.
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Bowman, D.M. (2017). The \(\varvec{{ Kepler}}\) Space Photometry Revolution. In: Amplitude Modulation of Pulsation Modes in Delta Scuti Stars. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-66649-5_2
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