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 The Nainital-Cape Survey: IV. A search for pulsational variability in 108 chemically peculiar stars Subject The topic of the resource Asteroseismology; Methods: observational; Stars: chemically peculiar; Stars: oscillations; Surveys Description An account of the resource The Nainital-Cape Survey is a dedicated ongoing survey program to search for and study pulsational variability in chemically peculiar (CP) stars to understand their internal structure and evolution. Aims. The main aims of this survey are to find new pulsating Ap and Am stars in the northern and southern hemisphere and to perform asteroseismic studies of these new pulsators. Methods. The survey is conducted using high-speed photometry. The candidate stars were selected on the basis of having Stromgren photometric indices similar to those of known pulsating CP stars. Results. Over the last decade a total of 337 candidate pulsating CP stars were observed for the Nainital-Cape Survey, making it one of the longest ground-based surveys for pulsation in CP stars in terms of time span and sample size. The previous papers of this series presented seven new pulsating variables and 229 null results. In this paper we present the light curves, frequency spectra and various astrophysical parameters of the 108 additional CP stars observed since the last reported results. We also tabulated the basic physical parameters of the known roAp stars. As a part of establishing the detection limits in the Nainital-Cape Survey, we investigated the scintillation noise level at the two observing sites used in this survey, Sutherland and Nainital, by comparing the combined frequency spectra stars observed from each location. Our analysis shows that both the sites permit the detection of variations of the order of 0.6 milli-magnitude (mmag) in the frequency range 1-4 mHz, Sutherland is on average marginally better. 2016 ESO. Creator An entity primarily responsible for making the resource Joshi S.; Martinez P.; Chowdhury S.; Chakradhari N.K.; Joshi Y.C.; Van Heerden P.; Medupe T.; Kumar Y.B.; Kuhn R.B. Source A related resource from which the described resource is derived Astronomy and Astrophysics, Vol-590 Publisher An entity responsible for making the resource available EDP Sciences Date A point or period of time associated with an event in the lifecycle of the resource 2016-01-01 Identifier An unambiguous reference to the resource within a given context <a href="https://doi.org/10.1051/0004-6361/201527242" target="_blank" rel="noreferrer noopener">https://doi.org/10.1051/0004-6361/201527242</a> <br /><br /><a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-84971635985&amp;doi=10.1051%2F0004-6361%2F201527242&amp;partnerID=40&amp;md5=a65b5a638ff41f47e3b5ab86bfdaf54a" target="_blank" rel="noreferrer noopener">https://www.scopus.com/inward/record.uri?eid=2-s2.0-84971635985&amp;doi=10.1051%2f0004-6361%2f201527242&amp;partnerID=40&amp;md5=a65b5a638ff41f47e3b5ab86bfdaf54a</a> Rights Information about rights held in and over the resource All Open Access; Bronze Open Access; Green Open Access Relation A related resource ISSN: 46361; CODEN: AAEJA 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 Joshi S., Aryabhatta Research Institute of Observational Sciences, Nainital, 263129, India; Martinez P., SpaceLab, Department of Electrical Engineering, University of Cape Town, Private Bag X3, Rondebosch, 7701, South Africa, South African Astronomical Observatory, PO Box 9, Observatory, 7935, South Africa; Chowdhury S., Department of Physics, Christ University, Hosur Road, Bangalore, Karnataka, 560029, India; Chakradhari N.K., School of Studies in Physics and Astrophysics, Pt Ravishankar Shukla University, Raipur, 492010, India; Joshi Y.C., Aryabhatta Research Institute of Observational Sciences, Nainital, 263129, India; Van Heerden P., South African Astronomical Observatory, PO Box 9, Observatory, 7935, South Africa; Medupe T., Department of Physics, University of the North-West, Private Bag X2046, Mmabatho, 2735, South Africa; Kumar Y.B., National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, China; Kuhn R.B., South African Astronomical Observatory, PO Box 9, Observatory, 7935, South Africa