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218 Figure. Abstract 219 Figure.219 Figure. Published on behalf of the European Society of Cardiology. All rights reserved. & The Author 2015. For permissions please email: [email protected]. European Heart Journal Cardiovascular Imaging Abstract Supplements – volume 16 supplement 1 May 2015 doi:10.1093/ehjci/jev050 Downloaded from https://academic.oup.com/ehjcimaging/article-abstrac...
Case-Based Session: Cases from Outside Europe: Friday 5 December 2014, 15:30-16:30 * Location: Agora
Empirical studies of static and dynamic diagrams have traditionally collected outcome data indicating the effectiveness of these depictions with respect to comprehension and learning. Because outcome measures alone provide limited insights as to why diagrams are or are not effective, there has been growing interest in studying how people process these depictions. In some cases, the aim of this ...
ing has been a goal of lighting researchers—and the broader lighting industry—for decades. The utility of the Commission Internationale de l’Eclairage’s (CIE’s) general color rendering index (Ra, commonly called CRI)1 has been demonstrated by its continued use for 50 years, but its limitations and deficiencies are becoming ever more prominent with the advent of solid-state lighting, which provi...
This paper presents a comprehensive examination of the X-ray continuum variability of the bright Seyfert 1 galaxy MCG–6-30-15. The source clearly shows the strong, linear correlation between rms variability amplitude and flux first seen in Galactic X-ray binaries. The high frequency power spectral density (PSD) of MCG–6-30-15 is examined in detail using a Monte Carlo fitting procedure and is fo...
We present results from fitting ionized disc models to three long ASCA observations of the Seyfert 1 galaxy MCG–6-30-15. All three datasets are well fit by a model consisting of ionized reflection from the inner region of the accretion disc (with twice solar Fe abundance) and a separate diskline component from farther out on the the disc. The diskline is required to fit the height of the observ...
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