First Post

Hello! My name is Kelly and I am an intern in the reference department this semester, which is very exciting. I was thrilled when I found out that I was going to be working here this semester. This is exactly what I wanted to do during my senior year, since next year I am planning on going to grad school for library science. But before I applied, I wanted to make sure I had some experience under my belt, and that I had some idea of what I was getting myself into. Which, as it turns out, I only had some idea of. Library science and reference are harder than I thought. There is a lot of technology involved as well as a thorough knowledge of research techniques and the library catalogue itself. It may look easy when you see a librarian finding a book or pulling up information, but it\u27s not. There\u27s a reason I have to get a degree to know how to do it. The more I work, the more excited I am to go to grad school and experience it myself. [excerpt

One Big Thing: Suffering as the Path to New Life in Crime and Punishment

After spending a whole semester reading and thinking about Dostoevsky, the main thing that has struck me about him is his treatment of the theme of suffering. Despite, and even through, his extremely complicated characters and events, he nevertheless focuses his novels, particularly Crime and Punishment, on presenting a nuanced yet unified picture of suffering. After a brief analysis of several of the relevant characters and plot points, his thoughts on what suffering does to and for the individual will be presented. In contrast to our culture’s almost idolization of suffering as an experience which gives one instant respect, authority, and a platform, Dostoevsky’s perspective is honest, informed, pragmatic, and thoroughly Christian

Evaluating the Mexico city policy: How US foreign policy affects fertility outcomes and child health in Ghana

US development assistance represents a significant source of funding for many population programs in poor countries. The Mexico City policy, known derisively as the global gag rule, restricts activities of foreign nongovernmental organizations (NGOs) that receive such assistance. The intent of the policy is to reduce the use of abortion in developing countries—a policy that is born entirely of US domestic politics and that turns on and off depending on the political party in power. I examine here whether the policy achieves its aim, and how the policy affects reproductive outcomes for women in Ghana. Employing a woman-by-month panel of pregnancies and woman fixed effects, I estimate whether a given woman is less likely to abort a pregnancy during two policy periods versus two nonpolicy periods. I find no evidence that any demographic group reduces the use of abortion as a result of the policy. On the contrary, rural women significantly increase abortions. This effect seems to arise from their increased rate of conception during these times. The policy-induced budget shortfalls reportedly forced NGOs to cut rural outreach services, reducing the availability of contraceptives in rural areas. The lack of contraceptives likely caused the observed 12 percent increase in rural pregnancies, ultimately resulting in about 200,000 additional abortions and between 500,000 and 750,000 additional unintended births. I find that these additional unwanted children have significantly reduced height and weight for age, relative to their siblings. Rather than reducing abortion, this policy increased pregnancy, abortion, and unintended births, resulting in more than a half-million children of significantly reduced nutritional status.abortion, child health, fertility, Foreign aid,

Tidally Driven Oscillations in KIC 4544587: a δ Scuti Binary System

Binary modelling techniques and frequency analysis have been applied to the Kepler photometric observations of KIC 4544587 to determine information about the orbital characteristics, individual components and tidal interactions. The system contains an early A-type δ Scuti variable, which pulsates in both pressure and gravity modes, and a late F- to early G-type star, which is possibly a solar-like oscillator. The Wilson-Devinney code was used to model the Quarter 3.2 data and PHOEBE was used to model the Quarter 7 data; the results of these two methods were then compared. Using PHOEBE the rate of apsidal advance was determined to be 0.0001179(1) rad d-1, which gives 145.9(1) yr for a complete precession. Subsequently the binary model light curve was subtracted from the original data and frequency analysis was performed on the residuals. Fifteen frequencies were identified that are harmonics of the orbital period, 9 of which are in the g mode regime and 6 in the p mode regime. It was concluded that these frequencies are not an artifact of the model fit and thus are a signature of tidal resonance. It was also determined that many of the frequencies in the p mode regime are separated from the two dominant p modes by a multiple of the orbital frequency; six of the identified modes demonstrate this separation to an accuracy of 3 σ. As they are not orbital harmonics, the origin of these frequencies remains unknown. Currently we know of no other star demonstrating these characteristics