Research Scientist I, S3
Apply now
Job no: 504117
Department: Center for Space Plasma & Aeronomic Research
Work type: Staff Full-time Exempt
Location: Alabama
Categories: Research - Engineering
| Purpose of the Position: |
The Research Scientist will conduct astrophysical research at the postdoctoral level within the designated area of specialization, analyze XRISM data from AO1 program 12190, study the active galaxy NGC 7212, & publish results.
Duties/Responsibilities • Conduct astrophysical research at the postdoctoral level within the designated area of specialization. • Analyze and interpret X-ray observational data from the XRISM mission related to the active galactic nucleus in NGC 7212. • Complete data analysis and research activities associated with Research Program 12190, Cosmic Ray Spallation and the Enigmatic Extended Narrow Line Region of NGC 7212. • Characterize and evaluate the origins of X-ray emission through comparative analysis with Chandra X-ray Observatory data. • Investigate the influence of obscuring torus structures on observed X-ray emission characteristics. • Develop, apply, and assess phenomenological models of X-ray line emission. • Utilize physically motivated modeling techniques, including reflection models and thermal ionized plasma models, to interpret observational data as project priorities and timelines permit. • Interpret research findings, document results, and contribute to the advancement of astrophysical research objectives. • Collaborate with principal investigators and research team members to achieve project milestones and support sponsored research initiatives. • Prepare, write, and publish peer-reviewed astrophysical research papers based on the analysis and interpretation of observational data. • Analyze new and existing XRISM X-ray Observatory data collected from observations of the active galaxy NGC 7212. • Document and characterize the potential detection of highly ionized helium-like vanadium and evaluate its astrophysical significance. • Analyze and interpret X-ray emission and absorption features identified through XRISM Research Program 12190, Cosmic Ray Spallation and the Enigmatic Extended Narrow Line Region of NGC 7212. • Apply relevant physical models to characterize observed emission and absorption properties and constrain their underlying astrophysical processes. • Interpret research findings, prepare scientific manuscripts, and disseminate results through peer-reviewed publications and other scholarly communications. • Maintain accurate documentation of research methodologies, analytical procedures, and study results in accordance with scientific and sponsor requirements. • Collaborate with research team members to support project objectives and advance sponsored astrophysical research initiatives. • Conduct collaborative astrophysical research utilizing multiple astrophysical targets and data from NASA X-ray observatories, including polarimetric observations from IXPE. • Analyze and interpret observational data from IXPE and other NASA X-ray observatories to investigate black holes and other high-energy astrophysical phenomena. • Develop and submit scientific observing proposals to obtain new IXPE observations in support of sponsored research objectives. • Design observational strategies and research methodologies to advance the understanding of black holes and other energetic astrophysical systems. • Collaborate with interdisciplinary research teams to plan, execute, and disseminate findings from observational research projects. • Contribute to the development of innovative research initiatives and future observational programs that support the advancement of high-energy astrophysics.
|
| Minimum Requirements: |
• Master's degree or an equivalent combination of education and years of experience • 6 - 9 months full-time verifiable work experience • Previous analysis of XRISM data using relevant AGN models such as MYTorus. Previous X-ray work on NGC 7212. • Knowledge of MS Office Suite
|
| Desired Qualifications: |
• Ph.D. in Astronomy and Astrophysics preferred • 3 years of postdoctoral research in astrophysics using XRISM and IXPE. Multiple first-author black hole publications are desired. • Focus: X-ray study of supermassive black holes preferred • Collaboration with NASA scientists using XRISM and IXPE, studying black holes and neutron stars. Experience as PI of NASA X-ray observations is desired. • Previous IXPE proposal submissions. Familiarity with the NASA proposal review process, such as service on a panel for IXPE peer review preferred.
|
| Published Salary (if available): |
$68,151 - $69,000
|
Advertised: Central Daylight Time
Applications close: Central Daylight Time
Back to search results Apply now Refer a friend