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April 2, 2024: We release a new version of the seismic indices and granulation parameters extracted from red-giant stars observed by the Kepler and CoRoT mission. These new indices have been extracted after having identifying a problem in the pre-processing of the Kepler light-curves and by using a slightly improved version of the MLEUP method. For more details see this release note.

April 10, 2018: all the stellar indices (CoRoT+Kepler) have been re-generated and inserted again in the DB ; the changes mainly concern the uncertainties associated with each stellar indice, which have been corrected for biases as described in de Assis Peralta et al (2018, see Appendix A.2.2).
April 9, 2018: to be published soon "A new method for extracting seismic indices and granulation parameters: results for more than 20,000 CoRoT and Kepler red giants", de Assis Peralta, Samadi, Michel, 2018, in Astronomische Nachrichten. If you use these data please refers to that paper.
November 25, 2016: A truncation error, affecting some of the values returned in the CSV file, has been corrected
November 8, 2016: Opening of the database (see this official announcement)

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Release note 2 April 2024 (PDF - 768.8 kb)

We describe in this note a new release of the seismic indices and granulation parameters extracted from red-giant stars observed by the Kepler and CoRoT mission. These new indices have been extracted after having identifying a problem in the pre-processing of the Kepler light-curves and by using a slightly improved version of the MLEUP method (de Assis Peralta et al. 2016).