Testing a Computational Model of Rhythm Perception Using Polyrhythmic Stimuli

By Vassilis Angelis, Simon Holland, Paul J. Upton, Martin Clayton. 2013

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In Cognitive Neuroscience

Citations in the corpus

The Second APOKASC Catalog: The Empirical Approach (2018, methodology): “The SDSS-IV and APOKASC-2 Samples The full APOGEE data sample we use was observed in SDSS-III (but analyzed in SDSS-IV) and contains 11,877 stars.”
Modern stellar spectroscopy caveats (2019, unknown): “Large surveys such as APOGEE (Eisenstein et al. 2011; Majewski et al. 2017) or the Gaia-ESO Public Spectroscopic Survey (GES; Gilmore et al. 2012; Randich et al. 2013), complemented by smaller surveys like OCCASO (Casamiquela et al. 2016, 2017) plus other independent studies and observational…”
The origin of accreted stellar halo populations in the Milky Way using APOGEE,Gaia, and the EAGLE simulations (2018, methodology): “The data employed in this paper come from the DR14 catalogue (Abolfathi et al. 2018), which comprises a re-reduction and analysis of APOGEE-1 data (from SDSS-III, Eisenstein et al. 2011), alongside a set of newly reduced and analysed observations from APOGEE-2 (taken as part of SDSS-IV, Blanton et a”
The Zwicky Transient Facility Catalog of Periodic Variable Stars (2020, methodology): “…in spectroscopic surveys—such as those undertaken with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST; Cui et al. 2012; Deng et al. 2012) and the Sloan Digital Sky Survey (SDSS; Eisenstein et al. 2011)—to reduce the systematic effects pertaining to the presence of variables.”
Discovery of 21 New Changing-look AGNs in the Northern Sky (2017, methodology): “The SDSS imaging survey scanned the sky in five filters, ugriz (Fukugita et al. 1996), covering 11,663 deg2 in SDSS-I/ II from 2000 to 2007 (Abazajian et al. 2009) and an additional 3,000 deg2 in SDSS-III in 2008.”