Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource Articles Article Faculty Publications -Articles Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource A study of pulsation &amp; rotation in a sample of A-K type stars in the Kepler field Subject The topic of the resource Stars: oscillations; Stars: rotation, starspots; Stars: variables; Stars: variables: solarlike; Stars: variables: ? Scuti Description An account of the resource We present the results of time-series photometric analysis of 15106 A-K type stars observed by the Kepler space mission. We identified 513 new rotational variables and measured their starspot rotation periods as a function of spectral type and discuss the distribution of their amplitudes. We examined the well-established period-color relationship that applies to stars of spectral types F5-K for all of these rotational variables and, interestingly, found that a similar period-color relationship appears to extend to stars of spectral types A7 to early-F too. This result is not consistent with the very foundation of the period-color relationship. We have characterized 350 new non-radial pulsating variables such as A- and F-type candidate ? Scuti, ? Doradus and hybrid stars, which increases the known candidate non-radial pulsators in the Kepler field significantly, by ?20%. The relationship between two recently constructed observables, Energy and Efficiency, was also studied for the large sample of non-radial pulsators, which shows that the distribution in the logarithm of Energy (log (En)) can be used as a potential tool to distinguish between the non-radial pulsators, to some extent. Through visual inspection of the light curves and their corresponding frequency spectra, we found 23 new candidate red giant solar-like oscillators not previously reported in the literature. The basic physical parameters such as masses, radii and luminosities of these solar-like oscillators were also derived using asteroseismic relations. 2018, The Author(s). Creator An entity primarily responsible for making the resource Chowdhury S.; Joshi S.; Engelbrecht C.A.; De Cat P.; Joshi Y.C.; Paul K.T. Source A related resource from which the described resource is derived Astrophysics and Space Science, Vol-363, No. 12 Publisher An entity responsible for making the resource available Springer Netherlands Date A point or period of time associated with an event in the lifecycle of the resource 2018-01-01 Identifier An unambiguous reference to the resource within a given context <a href="https://doi.org/10.1007/s10509-018-3480-1" target="_blank" rel="noreferrer noopener">https://doi.org/10.1007/s10509-018-3480-1</a> <br /><br /><a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85057811286&amp;doi=10.1007%2Fs10509-018-3480-1&amp;partnerID=40&amp;md5=1c5fa8759a99ee730ac9a5e1556a5166" target="_blank" rel="noreferrer noopener">https://www.scopus.com/inward/record.uri?eid=2-s2.0-85057811286&amp;doi=10.1007%2fs10509-018-3480-1&amp;partnerID=40&amp;md5=1c5fa8759a99ee730ac9a5e1556a5166</a> Rights Information about rights held in and over the resource All Open Access; Green Open Access; Hybrid Gold Open Access Relation A related resource ISSN: 0004640X Format The file format, physical medium, or dimensions of the resource Online Language A language of the resource English Type The nature or genre of the resource Article Coverage The spatial or temporal topic of the resource, the spatial applicability of the resource, or the jurisdiction under which the resource is relevant Chowdhury S., Nicolaus Copernicus Astronomical Center, Bartycka 18, Warsaw, 00-716, Poland, Department of Physics, CHRIST (Deemed to be University), Hosur Road, Bengaluru, 560029, Karnataka, India, Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital, 263002, India; Joshi S., Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital, 263002, India; Engelbrecht C.A., Department of Physics, University of Johannesburg, PO Box 524, Auckland Park, Johannesburg, 2006, South Africa; De Cat P., Royal Observatory of Belgium, Ringlaan 3, Brussel, 1180, Belgium; Joshi Y.C., Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital, 263002, India; Paul K.T., Department of Physics, CHRIST (Deemed to be University), Hosur Road, Bengaluru, 560029, Karnataka, India