Marshall University Music Department Presents a Jazz Ensemble II, Mr. Jeffrey Wolfe, Director

https://mds.marshall.edu/music_perf/1382/thumbnail.jp

Marshall University Music Department Presents a Jazz Ensemble II, Mr. Jeffrey Wolfe, Director

https://mds.marshall.edu/music_perf/1350/thumbnail.jp

Marshall University Music Department Presents Jazz Ensemble II, Mr. Jeffrey Wolfe, Director

https://mds.marshall.edu/music_perf/1718/thumbnail.jp

Marshall University Music Department Presents a Jazz Ensemble II, Mr. Jeffrey Wolfe, Director

https://mds.marshall.edu/music_perf/1663/thumbnail.jp

Marshall University Music Department Presents a Jazz Combos Recital

https://mds.marshall.edu/music_perf/1441/thumbnail.jp

Integrating Private Company Principles into a Government Department

In this session we present steps taken to improve the public image and employee culture at the Boone County Highway Department, including policies, processes, and strategies we implemented successfully and attempted changes that weren’t successful. We will discuss challenges we faced and the image we had to overcome at the onset of our transformation, as well as goals established in planning for the future of the department

Marshall University Music Department Presents the Marshall University Jazz Ensemble 12.0, Ed Bingham, director, with guest artist Jeff Wolfe, trumpet, assisted by Sean Parsons

https://mds.marshall.edu/music_perf/1447/thumbnail.jp

Marshall University Music Department Presents the MU Jazz Combo Concert

https://mds.marshall.edu/music_perf/1515/thumbnail.jp

Measurement of the Spatial Cross-Correlation Function of Damped Lyman Alpha Systems and Lyman Break Galaxies

We present the first spectroscopic measurement of the spatial cross-correlation function between damped Lyman alpha systems (DLAs) and Lyman break galaxies (LBGs). We obtained deep u'BVRI images of nine QSO fields with 11 known z ~ 3 DLAs and spectroscopically confirmed 211 R < 25.5 photometrically selected z > 2 LBGs. We find strong evidence for an overdensity of LBGs near DLAs versus random, the results of which are similar to that of LBGs near other LBGs. A maximum likelihood cross-correlation analysis found the best fit correlation length value of r_0 = 2.9^(+1.4)_(-1.5) h^(-1)Mpc using a fixed value of gamma = 1.6. The implications of the DLA-LBG clustering amplitude on the average dark matter halo mass of DLAs are discussed.Comment: 12 pages, 2 figures, accepted for publication in Astrophysical Journal Letter