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"Boss, Jack Forrest"
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Analyzing the Music of Living Composers (and Others)
Analyzing the Music of Living Composers (and Others) is a collection of essays that grew out of the 2010 annual meeting of the West Coast Conference of Music Theory and Analysis. The stated purpose was to apply traditional music-analytic techniques, as well as new, innovative techniques, to describing the music of composers of the late 20th and early 21st centuries. The goal was to take steps toward making the music of our time a bit less impenetrable for our colleagues, students and other li.
eBook
Form and Process in Music, 1300-2014
Form and Process in Music, 1300-2014: An Analytic Sampler draws together papers delivered at the 2014 meeting of the West Coast Conference of Music Theory and Analysis. The conference spanned an unusually wide spectrum of musical styles, including papers on European twelve-tone music after the Second World War, fourteenth-century music, pop music and jazz, the music of living composers, narrative and characterization, and the history of music theory. The title of the book reflects the large span of musical cultures that are represented within, but also accounts for the common thread through all of these essays, a strong emphasis on understanding the forms and processes of music through analysis. The reader will find within it a compendium of analytic techniques for numerous musical styles.
eBook
Schenker Studies 2
\"Schenker Studies 2\" edited by Carl Schachter and Hedi Siegel is reviewed.
Book Review
Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler
We report the distribution of planets as a function of planet radius (R_p), orbital period (P), and stellar effective temperature (Teff) for P < 50 day orbits around GK stars. These results are based on the 1,235 planets (formally \"planet candidates\") from the Kepler mission that include a nearly complete set of detected planets as small as 2 Earth radii (Re). For each of the 156,000 target stars we assess the detectability of planets as a function of R_p and P. We also correct for the geometric probability of transit, R*/a. We consider first stars within the \"solar subset\" having Teff = 4100-6100 K, logg = 4.0-4.9, and Kepler magnitude Kp < 15 mag. We include only those stars having noise low enough to permit detection of planets down to 2 Re. We count planets in small domains of R_p and P and divide by the included target stars to calculate planet occurrence in each domain. Occurrence of planets varies by more than three orders of magnitude and increases substantially down to the smallest radius (2 Re) and out to the longest orbital period (50 days, ~0.25 AU) in our study. For P < 50 days, the radius distribution is given by a power law, df/dlogR= k R^ This rapid increase in planet occurrence with decreasing planet size agrees with core-accretion, but disagrees with population synthesis models. We fit occurrence as a function of P to a power law model with an exponential cutoff below a critical period P_0. For smaller planets, P_0 has larger values, suggesting that the \"parking distance\" for migrating planets moves outward with decreasing planet size. We also measured planet occurrence over Teff = 3600-7100 K, spanning M0 to F2 dwarfs. The occurrence of 2-4 Re planets in the Kepler field increases with decreasing Teff, making these small planets seven times more abundant around cool stars than the hottest stars in our sample. [abridged]
Paper