Student Research Assistant- Pool

90%- Research and Instrumentation Development

• Conduct advanced research focused on the design measurement and calibration of scientific instruments used in cosmic-ray and neutrino detection.
• Responsibilities include developing experimental setups analyzing data troubleshooting equipment and ensuring precision in calibration processes to optimize detector sensitivity.

5%- Team Collaboration and Meetings

• Attend regular research team meetings to share progress discuss technical challenges and contribute to collaborative problem-solving.
• Provide input on experimental design and project planning.

5%- Presentation and Interpretation of Results

• Prepare and deliver presentations of research findings to internal teams and external collaborators.
• Interpret experimental data draft technical reports and contribute to publications or conference presentations.

Disclaimer
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Work Schedule
Up to 20 hours per week.

Contact Information to Applicants
Dave Besson

1. CompletedIntroductory College Physics coursework or equivalent as indicated on application materials.

1. Prior experience coding in C and/or python familiarity with linux and shell scripting languages as indicated on application materials.

This role will investigate techniques for calibrating and optimizing the sensitivity of cosmic-ray detector facilities based on measurements of radio-frequency signals generated by interactions of cosmic rays with ice molecules.

For the past three decades the KU particle astrophysics program has pursued the first-ever detection of ultra-high-energy cosmic neutrinos through radio-wave signals produced by neutrino interactions with polar ice. Current active experiments include ARA ARIANNA and PUEO in Antarctica as well as RNO-G and RET in Greenland. KU will also play a key role in the upcoming IceCube-Gen2 experiment at the South Pole.

Our research encompasses all aspects of these experiments including:
a) design measurement and calibration of instrumentation used to detect ultra-high-energy neutrinos;
b) measurement of the radio-frequency transmission properties of cold polar ice;
c) calibration of radio-frequency instrumentation both prior to and following deployment; and
d) direct searches for cosmic rays using radio techniques.

In addition we participate in astrobiological initiatives that explore correlations between cosmic-ray exposure and organismal metabolism. The hired individual will be expected to contribute to one or more of these efforts.

Additional Candidate Instruction
A complete application includes a cover letter and a resume or CV. Apply online and submit a letter describing your qualifications for this position. A review of applications will continue until qualified candidates are identifiedthrough May 13th 2026. Anticipated start date is as soon as possible. Only complete applications will be considered.

Position Requirements
During the semester term of the appointment the student hourly must be enrolled in no fewer than 6 credit hours. For summer periods the student hourly must: (1) have been enrolled in no less than 6 hours in the past spring semester or (2) be pre-enrolled in the upcoming fall semester in no less than 6 hours or (3) be enrolled in summer session or (4) be admitted to study in the upcoming fall semester. Student Hourlies may be undergraduate or graduate students. (Exceptions granted for GRA/GTA/GA appointments DO NOT apply to Student Hourly appointments).

Employment Conditions
(1) Student employees are not eligible for remote work arrangements unless an exception is approved by the unit leadership and HR.

(2) This is an hourly/non-exempt position. A student employee cannot hold an hourly/non-exempt position and a salaried/exempt graduate or undergraduate position (GRA/GTA/GA/RUA/RGA) concurrently.