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dc.contributor.authorFiguera Jaimes, R.
dc.contributor.authorBramich, D. M.
dc.contributor.authorSkottfelt, J.
dc.contributor.authorKains, N.
dc.contributor.authorJørgensen, U. G.
dc.contributor.authorHorne, K.
dc.contributor.authorDominik, M.
dc.contributor.authorAlsubai, K. A.
dc.contributor.authorBozza, V.
dc.contributor.authorCalchi Novati, S.
dc.contributor.authorCiceri, S.
dc.contributor.authorD'Ago, G.
dc.contributor.authorGalianni, P.
dc.contributor.authorGu, S.-H.
dc.contributor.authorHarpsøe, K. B. W.
dc.contributor.authorHaugbølle, T.
dc.contributor.authorHinse, T. C.
dc.contributor.authorHundertmark, M.
dc.contributor.authorJuncher, D.
dc.contributor.authorKorhonen, H.
dc.contributor.authorMancini, L.
dc.contributor.authorPopovas, A.
dc.contributor.authorRabus, M.
dc.contributor.authorRahvar, S.
dc.contributor.authorScarpetta, G.
dc.contributor.authorSchmidt, R. W.
dc.contributor.authorSnodgrass, C.
dc.contributor.authorSouthworth, J.
dc.contributor.authorStarkey, D.
dc.contributor.authorStreet, R. A.
dc.contributor.authorSurdej, J.
dc.contributor.authorWang, X.-B.
dc.contributor.authorWertz, O.
dc.identifier.citationFiguera Jaimes , R , Bramich , D M , Skottfelt , J , Kains , N , Jørgensen , U G , Horne , K , Dominik , M , Alsubai , K A , Bozza , V , Calchi Novati , S , Ciceri , S , D'Ago , G , Galianni , P , Gu , S-H , Harpsøe , K B W , Haugbølle , T , Hinse , T C , Hundertmark , M , Juncher , D , Korhonen , H , Mancini , L , Popovas , A , Rabus , M , Rahvar , S , Scarpetta , G , Schmidt , R W , Snodgrass , C , Southworth , J , Starkey , D , Street , R A , Surdej , J , Wang , X-B & Wertz , O 2016 , ' Exploring the crowded central region of ten Galactic globular clusters using EMCCDs : variable star searches and new discoveries ' , Astronomy & Astrophysics , vol. 588 , A128 , pp. 1-22 .
dc.identifier.otherBibCode: 2016A&A...588A.128F
dc.identifier.otherORCID: /0000-0002-3202-0343/work/75996707
dc.description.abstractAims: We aim to obtain time-series photometry of the very crowded central regions of Galactic globular clusters; to obtain better angular resolution than has been previously achieved with conventional CCDs onground-based telescopes; and to complete, or improve, the census of the variable star population in those stellar systems. Methods: Images were taken using the Danish 1.54-m Telescope at the ESO observatory at La Silla in Chile. The telescope was equipped with an electron-multiplying CCD, and the short-exposure-time images obtained (ten images per second) were stacked using the shift-and-add technique to produce the normal-exposure-time images (minutes). Photometry was performed via difference image analysis. Automatic detection of variable stars in the field was attempted.Results: The light curves of 12541 stars in the cores of ten globular clusters were statistically analysed to automatically extract the variable stars. We obtained light curves for 31 previously known variable stars (3 long-period irregular,2 semi-regular, 20 RR Lyrae, 1 SX Phoenicis, 3 cataclysmic variables, 1W Ursae Majoris-type and 1 unclassified) and we discovered 30 new variables (16 long-period irregular, 7 semi-regular, 4 RR Lyrae, 1 SX Phoenicis and 2 unclassified). Fluxes and photometric measurements for these stars are available in electronic form through the Strasbourg astronomical Data Center.
dc.relation.ispartofAstronomy & Astrophysicsen
dc.subjectBlue stragglersen
dc.subjectGalaxies: star clusters: generalen
dc.subjectGlobular clusters: generalen
dc.subjectStars: variables: RR Lyraeen
dc.subjectNovae, cataclysmic variablesen
dc.subjectInstrumentation: high angular resolutionen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleExploring the crowded central region of ten Galactic globular clusters using EMCCDs : variable star searches and new discoveriesen
dc.typeJournal articleen
dc.contributor.sponsorThe Royal Societyen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.description.statusPeer revieweden
dc.identifier.grantnumberUF100010 / UF130581en

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