Wavefront Correction and Photometry for Supernova Observations
Major
Physics
Second Major
Art, BA
Submission Type
Poster
Area of Study or Work
Physics
Faculty Advisor
Gabe Spalding
Expected Graduation Date
2027
Location
CNS Atrium
Start Date
4-13-2024 11:15 AM
End Date
4-13-2024 12:30 PM
Abstract
The study and identification of Supernovas rely heavily on the implementation of adaptive optics and photometry. Research on this specific astrological event is extremely significant in advancing discoveries in the realm of the life cycle of stars and the macro-world of space. This can lead to further understanding of the formation and behavior of neutron stars and black holes. Before requesting access to multi-million-dollar equipment, we are engaging in relevant skill building, using two distinct types of affordable components. We plan to develop a photometry system for use at our on-campus observatory, for analysis of the luminosity of observable supernovas. Additionally, we aim to utilize liquid-crystal-based devices to learn about the kinds of wavefront correction relevant to astronomical adaptive optics and to larger-scale cosmological observations.
Wavefront Correction and Photometry for Supernova Observations
CNS Atrium
The study and identification of Supernovas rely heavily on the implementation of adaptive optics and photometry. Research on this specific astrological event is extremely significant in advancing discoveries in the realm of the life cycle of stars and the macro-world of space. This can lead to further understanding of the formation and behavior of neutron stars and black holes. Before requesting access to multi-million-dollar equipment, we are engaging in relevant skill building, using two distinct types of affordable components. We plan to develop a photometry system for use at our on-campus observatory, for analysis of the luminosity of observable supernovas. Additionally, we aim to utilize liquid-crystal-based devices to learn about the kinds of wavefront correction relevant to astronomical adaptive optics and to larger-scale cosmological observations.