Session
2024 Poster Session
Location
Salt Lake Community College Westpointe Campus, Salt Lake City, UT
Start Date
5-6-2024 9:55 AM
Description
We are using Surface Brightness Fluctuations (SBF) to measure distances to giant elliptical galaxies using the Hubble Space Telescope (HST) and James Webb Space Telescope (JWST). These distance measurements will be used to better define the Hubble Constant, and hopefully help resolve the Hubble tension crisis in cosmology. Part of SBF requires a knowledge of the colors of the galaxies to be studied in order to account for variations in age and composition of the stars contained within. To this end, we are using PanSTARRS and DECam data to determine the optical g-z color (464 nm-900 nm) values for galaxies out to 300 million light years.
Correcting Surface Brightness Fluctuation Distances for Stellar Populations
Salt Lake Community College Westpointe Campus, Salt Lake City, UT
We are using Surface Brightness Fluctuations (SBF) to measure distances to giant elliptical galaxies using the Hubble Space Telescope (HST) and James Webb Space Telescope (JWST). These distance measurements will be used to better define the Hubble Constant, and hopefully help resolve the Hubble tension crisis in cosmology. Part of SBF requires a knowledge of the colors of the galaxies to be studied in order to account for variations in age and composition of the stars contained within. To this end, we are using PanSTARRS and DECam data to determine the optical g-z color (464 nm-900 nm) values for galaxies out to 300 million light years.