Search for high-amplitude δ Scuti and RR Lyrae stars in Sloan Digital Sky Survey Stripe 82 using principal component analysis

Süveges, M. ; Sesar, B. ; Váradi, M. ; Mowlavi, N. ; Becker, A. C. ; Ivezić, Ž. ; Beck, M. ; Nienartowicz, K. ; Rimoldini, L. ; Dubath, P. ; Bartholdi, P. ; Eyer, L.

In: Monthly Notices of the Royal Astronomical Society, 2012, vol. 424, no. 4, p. 2528-2550

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    We propose a robust principal component analysis framework for the exploitation of multiband photometric measurements in large surveys. Period search results are improved using the time-series of the first principal component due to its optimized signal-to-noise ratio. The presence of correlated excess variations in the multivariate time-series enables the detection of weaker variability. Furthermore, the direction of the largest variance differs for certain types of variable stars. This can be used as an efficient attribute for classification. The application of the method to a subsample of Sloan Digital Sky Survey Stripe 82 data yielded 132 high-amplitude δ Scuti variables. We also found 129 new RR Lyrae variables, complementary to the catalogue of Sesar et al., extending the halo area mapped by Stripe 82 RR Lyrae stars towards the Galactic bulge. The sample also comprises 25 multiperiodic or Blazhko RR Lyrae stars