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dc.contributor.authorScholz, Aleks
dc.contributor.authorWarwick, Ben
dc.contributor.authorvan Aalten, Thomas
dc.date.accessioned2022-10-25T23:36:21Z
dc.date.available2022-10-25T23:36:21Z
dc.date.issued2021-10
dc.identifier276580233
dc.identifier90d9cde6-045a-4724-aace-60669115ffde
dc.identifier.citationScholz , A , Warwick , B & van Aalten , T 2021 , ' The Fleming Survey : high-cadence survey for variable stars in the northern galactic plane ' , Research Notes of the AAS , vol. 5 , no. 10 , 245 . https://doi.org/10.3847/2515-5172/ac32bcen
dc.identifier.issn2515-5172
dc.identifier.otherJisc: c8b98db569954683bec80c2ac43f35dc
dc.identifier.otherpublisher-id: rnaasac32bc
dc.identifier.othermanuscript: ac32bc
dc.identifier.otherother: aas35494
dc.identifier.urihttps://hdl.handle.net/10023/26244
dc.description.abstractWe present first results from the Fleming Survey, a high-cadence search for variable stars in the northern Galactic Plane, conducted with the James Gregory Telescope in St Andrews (UK). After observing twelve fields, each over a timespan of 3–5 hr and with a cadence of 1 min, we identify 8 variable stars with clear periodic flux modulation in our lightcurves. Two of these are deemed to be δ Scuti pulsators, five are most likely eclipsing binaries. For most of our discoveries, the variability is known in the literature, but the exact period and shape of the lightcurve is not. This mini-survey demonstrates that high-cadence observations with small telescopes are a useful complement to ongoing and planned massive variability surveys.
dc.format.extent323980
dc.language.isoeng
dc.relation.ispartofResearch Notes of the AASen
dc.subjectDelta Cepheid variable starsen
dc.subjectSurveysen
dc.subjectW Ursae Majoris variable starsen
dc.subjectEclipsing binary starsen
dc.subjectAlgol variable starsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe Fleming Survey : high-cadence survey for variable stars in the northern galactic planeen
dc.typeJournal itemen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.identifier.doi10.3847/2515-5172/ac32bc
dc.description.statusPeer revieweden


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