1,919 research outputs found
Afro-Caribbean Immigrant Faculty Experiences in the American Academy: Voices of an Invisible Black Population
Afro-Caribbean immigrants have been an integral part of the history and shaping of the United States since the early 1900s. This current study explores the experiences of five Afro-Caribbean faculty members at traditionally White institutions of higher education. Despite the historical presence and influence of Afro-Caribbean communities and the efforts within education systems to address the needs of Afro-Caribbean constituents, Afro-Caribbean faculty members continue to be rendered indiscernible in higher education and to be frequently and erroneously perceived as African–Americans. The study examines the lived experiences of these individuals in the hegemonic White spaces they occupy at their institutions with both White and Black populations. Through their narratives, issues of stereotyping, microaggression, and isolation are addressed. The participants also offer solutions to address these issues by university administrators, department heads, faculty development professionals, diversity officers, policy makers, and other stakeholders. The voices in this study shed light on an overlooked, misunderstood, and under-researched population within our faculty ranks in the American Academy
Exploring the relationship between health-related fitness and biological CVD risk factors in Canadian young adult men and women
It is well known that physical inactivity leads to development of poor musculoskeletal health and obesity, two major modifiable risk factors for the development of Cardiovascular Disease (CVD; Eyre, Kahn, & Robertson, 2004). Unfortunately, physical inactivity is on the rise in Canada. Recent data from the Canadian Community Health Survey (Statistics Canada, 2005) suggests that 53.5% of Canadians are physically inactive, placing them at increased risk for CVD. In Canadian adults, gender differences in physical activity levels suggest that women appear to be less physically active than men (Heart and Stroke, 2003). The CVD risk associated with physical inactivity appears more substantial when, the relative risk for Coronary Artery Disease (CAD) associated with physical inactivity is equal to that of hypertension, high blood cholesterol, and cigarette smoking (Stewart, 2005)
DCC Digital Curation Manual: Instalment on Archiving Web Resources
Material on the Internet is transitory, fragile and ephemeral. Web archiving
represents a systematic attempt to bring stability to the information found in
websites
Mufasa: The assembly of the red sequence
We examine the growth and evolution of quenched galaxies in the Mufasa cosmo-
logical hydrodynamic simulations that include an evolving halo mass-based quench-
ing prescription, with galaxy colours computed accounting for line-of-sight extinc-
tion to individual star particles. Mufasa reproduces the observed present-day red
sequence quite well, including its slope, amplitude, and scatter. In Mufasa, the red
sequence slope is driven entirely by the steep stellar mass{stellar metallicity relation,
which independently agrees with observations. High-mass star-forming galaxies blend
smoothly onto the red sequence, indicating the lack of a well-de ned green valley at
M & 1010:5M . The most massive galaxies quench the earliest and then grow very
little in mass via dry merging; they attain their high masses at earlier epochs when
cold in
ows more e ectively penetrate hot halos. To higher redshifts, the red sequence
becomes increasingly contaminated with massive dusty star-forming galaxies; UVJ
selection subtly but e ectively separates these populations. We then examine the evo-
lution of the mass functions of central and satellite galaxies split into passive and
star-forming via UVJ. Massive quenched systems show good agreement with obser-
vations out to z 2, despite not including a rapid early quenching mode associated
with mergers. However, low-mass quenched galaxies are far too numerous at z . 1 in
Mufasa, indicating that Mufasa strongly over-quenches satellites. A challenge for
hydrodynamic simulations is to devise a quenching model that produces enough early
massive quenched galaxies and keeps them quenched to z = 0, while not being so
strong as to over-quench satellites; Mufasa only succeeds at the former.IS
FSSC Science Tools: Pulsar Analysis
This slide presentation reviews the typical pulsar analysis, giving tips for screening of the data, the use of time series analysis, and utility tools. Specific information about analyzing Vela data is reviewed
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