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UR: Phase Difference and Metallicity of RR Lyrae Variable Stars

UR: Phase Difference and Metallicity of RR Lyrae Variable Stars

by Guest | Nov 11, 2021 | Undergraduate Research

In the latest of our #UndergradResearch series, explore how Anna McElhannon is investigating the relationship between pulsation and metallicity in RR Lyrae stars!

UR: The Mystery of Orphan H II Regions: Where Are the Ionising Star Clusters?

UR: The Mystery of Orphan H II Regions: Where Are the Ionising Star Clusters?

by Guest | Oct 28, 2021 | Undergraduate Research

In the latest of our #UndergradResearch series, explore how Jia Wei Teh examines young star clusters and tries to match them to HII regions!

UR: Using Gaussian Processes to Study Exoplanet Transits and Stellar Variability Simultaneously

UR: Using Gaussian Processes to Study Exoplanet Transits and Stellar Variability Simultaneously

by Guest | Oct 27, 2021 | Undergraduate Research

In the latest of our #UndergradResearch series, discover how Larissa Palethorpe finds a way to get more information out of transit light curves.

UR: Acoustic Parameters as Discriminators of Wall Events in PICO Dark Matter Search Data

UR: Acoustic Parameters as Discriminators of Wall Events in PICO Dark Matter Search Data

by Guest | Oct 26, 2021 | Undergraduate Research

In the latest of our #UndergradResearch series, discover how Lucia Volkova has been working with PICO to improve bubble chambers, one possible way to detect dark matter.

UR: Quick–LOOK: Pulsar Data!

UR: Quick–LOOK: Pulsar Data!

by Guest | Sep 23, 2021 | Undergraduate Research

In the latest of our #UndergradResearch series, read about Katherine Zine and Blaise Veres’ work with NANOGrav’s Quicklook software, which allows them to quickly look at pulsar observations

UR: High Mass-Ratio Binary Populations in Galactic Open Clusters

UR: High Mass-Ratio Binary Populations in Galactic Open Clusters

by Guest | Sep 20, 2021 | Undergraduate Research

In our latest #UndergradResearch post, Naman Joshi investigated what fraction of binary stars have a high difference in mass between them.

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