Navigating a Music Career in Higher Education

Author(s):  
Colleen M. Conway

This final chapter examines the tenure and promotion process and provides sample paperwork from the School of Music, Theatre & Dance at the University of Michigan with details regarding rank and eligibility, promotion guides for teaching, promotion guidelines for scholarship, research and creative activity, and promotion guidelines for local, state, regional, national, and international service. Rules for deliberation and voting are shared including details about internal and external reviews and student evaluations. Instructions for the submission of paperwork including CVs, statements of teaching, research, and service and summaries of student evaluations are provided. Questions for discussion and final activities assist readers in considering the University of Michigan documents in relation to their home institution.

ICONI ◽  
2019 ◽  
pp. 149-158
Author(s):  
Joseph Pehrson ◽  

Joseph Pehrson is a well-known New York-based composer. He studied at the Eastman School of Music and the University of Michigan. He has been active in promoting contemporary music in New York, having been a co-director of the “Composers’ Concordance” concert organization from 1984 to 2011. Pehrson has written music in various styles, including neoclassical and avant-garde, microtonal music. The latter includes electronic compositions with and without solo instruments, which he wrote in the decade of the 2000s. He has delved very deeply into microtonal theory and has written compositions for various unusual and non-standard microtonal scales, such as the 21-note to the octave scale. The following is a transcript of Joseph Pehrson’s presentation at the Theremin Center, which was the Moscow Conservatory’s electronic studio in the 1990s and 2000s.


1979 ◽  
Vol 46 ◽  
pp. 96-101
Author(s):  
J.A. Graham

During the past several years, a systematic search for novae in the Magellanic Clouds has been carried out at Cerro Tololo Inter-American Observatory. The Curtis Schmidt telescope, on loan to CTIO from the University of Michigan is used to obtain plates every two weeks during the observing season. An objective prism is used on the telescope. This provides additional low-dispersion spectroscopic information when a nova is discovered. The plates cover an area of 5°x5°. One plate is sufficient to cover the Small Magellanic Cloud and four are taken of the Large Magellanic Cloud with an overlap so that the central bar is included on each plate. The methods used in the search have been described by Graham and Araya (1971). In the CTIO survey, 8 novae have been discovered in the Large Cloud but none in the Small Cloud. The survey was not carried out in 1974 or 1976. During 1974, one nova was discovered in the Small Cloud by MacConnell and Sanduleak (1974).


2006 ◽  
Vol 1 (9) ◽  
pp. 601
Author(s):  
Tonia J. Buchholz ◽  
Bruce Palfey ◽  
Anna K. Mapp ◽  
Gary D. Glick

Skull Base ◽  
2007 ◽  
Vol 17 (S 2) ◽  
Author(s):  
P. Ward ◽  
Lawrence Marentette

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