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Saskia Hekker

Researcher at Max Planck Society

Publications -  74
Citations -  3793

Saskia Hekker is an academic researcher from Max Planck Society. The author has contributed to research in topics: Stars & Asteroseismology. The author has an hindex of 25, co-authored 74 publications receiving 3042 citations. Previous affiliations of Saskia Hekker include Aarhus University.

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The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra

Romina Ahumada, +345 more
- 25 Jun 2020 - 
TL;DR: The most recent data release from the Sloan Digital Sky Surveys (SDSS-IV) is DR16 as mentioned in this paper, which is the fourth and penultimate from the fourth phase of the survey.
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The Thirteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey MApping Nearby Galaxies at Apache Point Observatory

Franco D. Albareti, +336 more
- 05 Aug 2016 - 
TL;DR: Data Release 13 (DR13) as mentioned in this paper is the first data release from SDSS-IV, which contains new data, reanalysis of existing data sets and, like all SDSs data releases, is inclusive of previously released data.
Journal ArticleDOI

The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra

Romina Ahumada, +312 more
- 05 Dec 2019 - 
TL;DR: The most recent data release from the Sloan Digital Sky Surveys (SDSS-IV) is DR16 as discussed by the authors, which is the fourth and penultimate from the fourth phase of the survey.
Journal ArticleDOI

Asteroseismology of the open clusters NGC 6791, NGC 6811, and NGC 6819 from nineteen months of Kepler photometry

Enrico Corsaro, +21 more
- 17 May 2012 - 
TL;DR: In this paper, the authors studied solar-like oscillations in 115 red giants in the three open clusters NGC 6791, NGC 6811, and NGC6819, based on photometric data covering more than 19 months with NASA's Kepler space telescope.
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Kepler-21b: A 1.6REarth Planet Transiting the Bright Oscillating F Subgiant Star HD 179070

Steve B. Howell, +65 more
- 09 Dec 2011 - 
TL;DR: In this paper, the authors present Kepler observations of the bright (V=8.3), oscillating star HD 179070, which reveal that the star is orbited every 2.8 days by a small, 1.6 R_Earth object.