Milky Way over the Atacama Desert

Time-series and observational data

Scientific Data Processing

A connected body of work spanning space-telescope photometry, time-series analysis, Fourier methods and spectroscopic preparation.

  • Data
  • Software
4,000+stellar light curves analysed
90objects selected for closer investigation
70+spectra prepared for analysis

01 / Context

Problem

Large observational datasets only become useful after consistent extraction, quality control, candidate selection and domain-specific analysis.

02 / Scope

My responsibility

I processed and analysed space-telescope data, including light curves from NASA's TESS mission, reduced the candidate set and prepared observational material for scientific interpretation.

03 / System

How it works

A deliberately simplified view of system boundaries and data movement.

Scientific data flow from space telescope observations and spectra through quality control and Fourier analysis to selected objects.
  1. 01Space telescope data and spectra
  2. 02Extraction and quality control
  3. 03Time-series and Fourier analysis
  4. 04Candidate selection
  5. 05Scientific interpretation

04 / Delivery

What I built

  • Processed and analysed the full stellar light-curve dataset.
  • Reduced the dataset to a scientifically focused candidate set.
  • Applied Fourier analysis to identify and characterise variability.
  • Prepared spectroscopic material for analysis.
  • Built and maintain lcView, a Python workbench integrating native C and Fortran engines for light-curve analysis.

05 / Decisions

Constraints and trade-offs

  • Automated screening provides scale, while final candidate selection still requires scientific judgement.
  • Combining datasets with different cadence and baselines requires careful separation of comparable and complementary evidence.

06 / Tools

Project stack

The technologies used across the system, grouped by the job they perform.

Application

Scientific computing

Native code and quality