The Postdoctoral Research Associate will conduct scientific research using James Webb Space Telescope (JWST) and Hubble Space Telescope (HST) multi-band imaging data to investigate how young, massive stars obscure older stellar populations in integrated-light studies of the early universe, a phenomenon known as “outshining.” The research will focus on understanding and calibrating outshining bias through detailed analysis of stellar populations in low-redshift analogs of high-redshift galaxies, using new and archival JWST and HST observations. The position will work closely with the Principal Investigator of a joint JWST-HST program and collaborate with NOIRLab researchers and a U.S.-based research team with expertise in the low- and high-redshift universe. Based at NSF NOIRLab’s Tucson headquarters, the role offers opportunities for scientific collaboration and engagement with the broader NOIRLab and Steward Observatory research communities. The position is set to start in Fall 2027. The successful candidate will analyze resolved stellar populations and spectral energy distributions, derive star formation histories, develop methods for emulating high-redshift observations, and produce science-ready data products. They will lead and collaborate on interpreting and communicating research findings through peer-reviewed publications and presentations. A PhD in Astronomy, Physics, Astrophysics, or a closely related field is required by the appointment start date.
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Job Type
Full-time
Career Level
Senior
Education Level
Ph.D. or professional degree