Postdoc-UCSB Physics Dept. (Galaxy Evolution)/Casey Research Group
University of California - Santa Barbara | |
United States, California, Santa Barbara | |
1021 Anacapa Street (Show on map) | |
Dec 19, 2024 | |
Position overview
Salary range:
A reasonable estimated full-time rate for this position at 100% time is $66,737 to $80,034/ year. Percent time:
100 Anticipated start:
Negotiable and should be by either summer 2025 or fall 2025. Position duration:
The initial appointment will be for two years with the expectation of renewal for a third year contingent upon satisfactory performance. Application Window Open date: December 19, 2024 Next review date: Friday, Jan 31, 2025 at 11:59pm (Pacific Time) Final date: Thursday, Dec 18, 2025 at 11:59pm (Pacific Time) Position description The Department of Physics at the University of California, Santa Barbara invites applications for 1-2 postdoctoral researchers to join UCSB's engaging and diverse astronomy group. The successful applicant(s) will work in collaboration with Prof. Caitlin Casey on a variety of observational datasets and projects spanning JWST (especially focused on, though not limited to the COSMOS-Web Survey), ALMA gas and dust observations, and Keck spectroscopy. The themes will span massive galaxies in the Universe's first Gyr, early star formation and AGN, galaxy clustering and large scale structure, and dust and gas at high-z. Applicants with experience in observational extragalactic astrophysics are encouraged to apply; those with expertise in optical/near-infrared (OIR) image analysis, OIR spectroscopy, sub/millimeter/radio astronomy, or SED fitting may be particularly well suited for the position(s). The department is especially interested in candidates who can contribute to the diversity and excellence of the academic community through research, teaching and service as appropriate to the position. Qualifications Basic qualifications
(required at time of application)
Applicants must have completed all requirements for Ph.D. (or equivalent), except the dissertation, at the time of application. The Ph.D. is expected to be in the fields of Physics, Astronomy, or closely related field. Additional qualifications
(required at time of start)
The candidate must have received their Ph.D. in the fields of Physics, Astronomy, or closely related field by the time the appointment begins. Preferred qualifications
It is preferred that candidates have 2-3 years of experience in observational extragalactic astrophysics (including graduate-level research) . Those with expertise in optical/near-infrared (OIR) image analysis, OIR spectroscopy, sub/millimeter/radio astronomy, or SED fitting may be particularly well suited for the position(s). Application Requirements Document requirements
Reference requirements
Please enter the contact information for your references (name, email address, phone number) and then trigger a solicitation in the system for the letters of recommendation. Apply link: https://recruit.ap.ucsb.edu/JPF02904 Help contact: erickajames@ucsb.edu About UC Santa Barbara The University of California is an Equal Opportunity/Affirmative Action Employer. All qualified applicants will receive consideration for employment without regard to race, color, religion, sex, sexual orientation, gender identity, national origin, disability, age or protected veteran status. For the University of California's Affirmative Action Policy please visit: https://policy.ucop.edu/doc/4010393/PPSM-20. For the University of California's Anti-Discrimination Policy, please visit: https://policy.ucop.edu/doc/1001004/Anti-Discrimination. As a condition of employment, you will be required to comply with the University of California Policy on Vaccination Programs, as may be amended or revised from time to time. Federal, state, or local public health directives may impose additional requirements. Job location Santa Barbara, CA
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