Tenure-Track Assistant Professor Position in Astronomy

The Department of Astronomy at the University of Texas at Austin invites applications for a tenure-track faculty position at the Assistant Professor level to begin in August 2026. We welcome applications from candidates in all fields of astronomy and we are open to observers, theorists, and instrumentalists. The search will be at a junior tenure-track level, but outstanding candidates at more senior ranks may be considered.

Information on departmental and McDonald Observatory resources and research programs can be found at: https://astronomy.utexas.edu

UT Austin is a major founding partner in the consortium for the next-generation 25-m Giant Magellan Telescope (GMT: http://www.gmto.org). UT Austin faculty members have access to McDonald Observatory, which hosts the 10-m Hobby-Eberly Telescope equipped with instruments such as the VIRUS wide-field integral field spectrograph and the Habitable-zone Planet Finder (HPF) precision-RV spectrograph. McDonald also hosts the HJST 2.7-m telescope with the Immersion Grating Infrared Spectrograph (IGRINS), the 2.1-m and 0.8-m telescopes, and a node for the Las Cumbres Observatory (LCO) network. The UT Astronomy Program provides vibrant collaborative opportunities on large astronomical surveys, including the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) and numerous surveys using JWST, HST, TESS, and other national/international facilities. Computational resources include the Texas Advanced Computing Center (TACC: https://www.tacc.utexas.edu), which designs and operates some of the world’s most powerful computing resources, and is known for its leadership in high performance computing, visualization, big data analytics, and machine learning.

UT Austin hosts a broad range of Centers and interdisciplinary initiative, including the Center for Planetary Systems Habitability (CPSH), Cosmic Frontiers Center (CFC), Wootton Center for Astrophysical Plasma Physics (WCAPP), Weinberg Institute of Theoretical Physics, and the NSF-Simons AI Institute for Cosmic Origins (CosmicAI).

Applicants should have a Ph.D. in Astronomy, Physics, Planetary Science, or related fields. The primary selection criteria will be excellence and leadership in astrophysics research, as well as a commitment to excellence in teaching and supervision of undergraduate and graduate students. We particularly seek candidates who will lead transformational science with next-generation observational and computational facilities, and creatively utilize the resources of the Astronomy Department and McDonald Observatory. Applicants are encouraged to highlight throughout their application their relevant experiences and skillsets in supporting academic success of all students (e.g., their specific approaches for teaching, mentoring, research and /or scholarly work).