Universities Space Research Association

Visiting Assoc Scientist, Astronomy

Education, Government & Non-Profit
5 - 7 years of experience
Job Overview by Ladders

Qualifications

  • PhD in Physics, Astronomy, Astrophysics, or related field, or equivalent experience.
  • 5+ years of relevant experience in time-domain astronomy and signal analysis.
  • Strong understanding of quasi-periodic and periodic signal analysis.
  • Familiarity with Bayesian inference and gravitational-wave data analysis is a plus.
  • Experience with observation scheduling and campaign design is advantageous.

Responsibilities

  • Construct synthetic EM signals from EMRI trajectories and model QPEs as disk-crossing events.
  • Design and execute mock EM observing campaigns with varied parameters.
  • Apply non-parametric reconstruction methods to recover harmonic phase evolution from light curves.
  • Determine the minimum harmonics needed for effective signal capture under sparse conditions.
  • Identify optimal EM observing duration and cadence for gravitational-wave phase constraints.
  • Characterize effects of aliasing and sampling bias on signal recovery and propose mitigation strategies.
  • Translate research findings into practical recommendations for EM observing campaigns.
  • Contribute to open-source software development and documentation on GitHub.

Benefits

  • Opportunity for a one-year appointment with potential extension based on performance and funding.
  • Engagement in cutting-edge research in multi-messenger astronomy.
  • Collaboration with a team of experts in gravitational-wave science.
  • Access to professional development opportunities, including conferences and publications.
Full Job Description
USRA and the Science and Technology Institute are seeking a full-time Associate Scientist (Visiting) to join our team. The associate scientist will study the electromagnetic (EM) observing strategies that best constrain the gravitational-wave (GW) counterparts of Extreme Mass Ratio Inspirals (EMRIs) for LISA. Using quasi-periodic eruptions (QPEs) and quasi-periodic oscillations (QPOs) from active galactic nuclei as periodic EM signatures of EMRIs, the researcher will characterize how sampling cadence, observation duration, and data gaps limit the recovery of phase information, and determine the minimum EM observing investment needed to usefully anchor a gravitational-wave search - providing practical, telescope-time-limited guidance for planning future multi-messenger observing campaigns. This is a one-year appointment with the potential to extend to three years, contingent on funding and performance.

Essential Duties/Responsibilities:

  • Construct synthetic electromagnetic (EM) signals from EMRI trajectories intersecting a precessing accretion disk, modeling quasi-periodic eruptions (QPEs) as disk-crossing events, and calculate expected light curves for known QPE/QPO EMRI candidates
  • Design and run mock EM observing campaigns that systematically vary sampling cadence, observation duration, session length, and data gaps, treating each as a hyperparameter of the search
  • Apply a trans-dimensional, non-parametric reconstruction (adapted from BayesWaveVoices) to recover harmonic phase evolution from each mock light curve, and quantify how well the recovered phase anchors a matched gravitational-wave search
  • Use the Eryn trans-dimensional sampler to determine the minimum number of harmonics and spline knots needed to capture the periodic EM signal under realistic, sparse observing conditions
  • Perform model selection across observing-schedule hyperparameters to identify the minimum EM observing duration and cadence that yields a usable gravitational-wave phase constraint, given limited telescope time
  • Characterize how aliasing, spectral leakage, and irregular sampling bias phase and period recovery for QPE- and QPO-like periodic signals, and propose mitigation strategies informed by prior knowledge of signal morphology
  • Translate results into practical recommendations for scheduling EM observing campaigns (e.g., XMM-Newton, Chandra, NICER) in support of LISA multi-messenger EMRI searches
  • Contribute to open-source software development, testing, and documentation on GitHub, in line with the project's Open Science and Data Management Plan
  • Prepare results for publication in journals and present findings at national and international conferences, including within the LISA Consortium


Required Qualifications:

Education: PhD in Physics, Astronomy, Astrophysics, or a related field, or equivalent combination of education and experience.

Experience: Candidates with at least 5 years of experience performing this type of work are highly preferred. Prior experience with time-domain astronomy and analysis of quasi-periodic or periodic signals (e.g., QPEs, QPOs, or comparable variable/transient phenomena) is strongly preferred. Experience with observation scheduling, survey/cadence optimization, or the design of observing campaigns is a plus. Familiarity with Bayesian inference (e.g., MCMC, nested sampling) and gravitational-wave data analysis or LISA science is a plus but not required.

Knowledge, Skills & Abilities:

  • Strong understanding of time-domain astronomy, particularly the timing analysis of quasi-periodic and periodic X-ray or optical signals
  • Familiarity with sampling theory and its practical limitations: aliasing, spectral leakage, and the effects of irregular sampling and data gaps on period/phase recovery
  • Understanding of how electromagnetic phase information can be used to anchor or constrain the phase evolution of a gravitational-wave signal in a multi-messenger search
  • Familiarity with compact-object astrophysics and accretion-disk phenomenology (e.g., QPEs, QPOs, tidal disruption events) is a plus
  • Ability to design, run, and interpret simulation-based validation studies, including mock observing campaigns and their downstream effect on gravitational-wave parameter recovery
  • Experience writing and maintaining scientific software in a collaborative, open-source environment
  • Strong written and verbal communication skills for producing documentation and peer-reviewed publications


Technology:

  • Proficiency in Python; experience with MCMC/Bayesian sampling packages (e.g., Eryn, emcee, PTMCMC) is highly desirable
  • Familiarity with time-frequency/timing analysis tools (e.g., wavelet transforms such as WDM, Lomb-Scargle periodograms) for quasi-periodic signals
  • Familiarity with gravitational-wave software ecosystems (e.g., FEW / Fast EMRI Waveforms, BayesWave, LISA response and noise-curve tools) sufficient to connect EM phase reconstruction to a GW phase-anchoring pipeline
  • Experience with version control (Git/GitHub) and open-source software development practices


Working Conditions: This job operates in a professional office environment. This role routinely uses standard office equipment such as computers, phones, photocopiers, etc. extensive online usage. This is largely a sedentary role.

Travel: None.

Applicants should apply to the posting at Home | USRA Careers and include a letter of interest, resume, or curriculum vitae. Additional information on USRA can be found at Home | USRA

About Universities Space Research Association

Universities Space Research Association (USRA) is a nonprofit corporation that provides research and development services to government and industry customers. The company specializes in space science and technology, earth science, and aerospace engineering. USRA was founded in 1969 by a group of universities and is headquartered in Columbia, Maryland. The company operates research centers and institutes across the United States, including the Lunar and Planetary Institute, the Earth from Space Institute, and the Center for Space Plasma and Aeronomic Research.
Learn more about Universities Space Research Association
Size
500 employees
Industry

Similar Jobs

More Jobs at Universities Space Research Association

More Education, Government & Non-Profit Jobs

Find similar Visiting Assoc Scientist, Astronomy jobs: