Physical Sciences and Mathematics Commons^™

Investigating Drought Response And Paleoclimate Potential Of A New Network Of White Oak Chronologies In Western Kentucky, Usa, Audrey J. Heichelbech, Maegen L. Rochner, Megan Gibson

Undergraduate Research Events

In Kentucky, historic and paleo-climate data are limited, and current understanding of long-term climate change in the state relies on instrumental data spanning only 1895-present. Proxy data are necessary to extend the temporal and spatial span of climate information. One potential proxy source for Kentucky is tree ring data, but currently, only four such datasets are publicly available on the International Tree Ring Data Bank (ITRDB). Archaeological and archival timber sources may help to fill in this gap. In the 1940s, Florence Hawley-Ellis, the first woman dendrochronologist, collected samples of white oak (Quercus alba L.) from four counties in western …

Clean & Fast Amide Couplings In Water, Nicklas Buckbinder, Sudripet Sharma, Sachin Handa

Undergraduate Research Events

EDC

(1-Ethyl-3-(3-dimethylaminopropyl)carbodiimide) is a carbodiimide that is well known reagent for the amide coupling reactions between an amine and carboxylic acid in the presence of a base. It is the commonly used coupling agent in industries because it produces a water-soluble urea byproduct, which can be easily removed by an aqueous work-up. However, our methodology, the desired amide product precipitates out of the reaction mixture, and no additional work-up is required.3 Using aqueous micelles of PS-750-M as a solvent dramatically increases the rate of reaction.2 The filtrate recovered can be recycled to perform several coupling runs after post-reaction manipulation.

Using Saoimage Ds9 & Hubble Space Telescope Data To Identify Globular Clusters In Ic 219, Emily Spicer, Alice Jacques, Benne Holwerda

Undergraduate Research Events

Globular clusters are tightly bound spherical clusters of stars located within the halo of elliptical and spiral galaxies. They are among the oldest stars found in a galaxy, and their presence and abundance in a galaxy’s halo offer insight on the age, composition, and formation of the galaxy.1 I used a Hubble Space Telescope (HST) image and SAOImage DS9, a powerful imaging tool used to analyze astronomical data, to identify the size and locate the position of globular cluster (GC) candidates in IC 219.