000002081 001__ 2081
000002081 005__ 20160701171658.0
000002081 0247_ $$2DOI$$a10.1093/mnras/stw716
000002081 037__ $$aASTROimport-238
000002081 100__ $$aMoretti, M. I.
000002081 245__ $$aThe VMC survey - XX. Identification of new Cepheids in the Small Magellanic Cloud
000002081 260__ $$c2016
000002081 520__ $$aWe present Ks-band light curves for 299 Cepheids in the Small Magellanic Cloud (SMC) of which 288 are new discoveries that we have identified using multi-epoch near-infrared photometry obtained by the VISTA survey of the Magellanic Clouds system (VMC). The new Cepheids have periods in the range from 0.34 to 9.1 d and cover the magnitude interval 12.9 = s> = 17.6 mag. Our method was developed using variable stars previously identified by the optical microlensing survey OGLE. We focus on searching new Cepheids in external regions of the SMC for which complete VMC Ks-band observations are available and no comprehensive identification of different types of variable stars from other surveys exists yet. 
000002081 700__ $$a Clementini, G.
000002081 700__ $$a Ripepi, V.
000002081 700__ $$a Marconi, M.
000002081 700__ $$a Rubele, S.
000002081 700__ $$a Cioni, M.-R. L.
000002081 700__ $$a Muraveva, T.
000002081 700__ $$a Groenewegen, M. A. T.
000002081 700__ $$a Cross, N. J. G.
000002081 700__ $$a Ivanov, V. D.
000002081 700__ $$a Piatti, A. E.
000002081 700__ $$a de Grijs, R.
000002081 773__ $$c1687-1697$$i2$$pMonthly Notices of the Royal Astronomical Society$$v459$$y2016
000002081 85642 $$ahttp://esoads.eso.org/abs/2016MNRAS.459.1687M
000002081 905__ $$apublished in
000002081 980__ $$aREFERD