Four Very Large Telescope Unit Telescopes on Cerro Paranal at twilight under a deep blue sky.

Time domain and archives

Astronomy

Transit timing, archive photometry, and the instrumentation that connects a photon count to a physical model.

Very Large Telescope at twilight, Cerro Paranal. Photo: ESO/B. Tafreshi (twanight.org), CC BY 4.0.

The question

Can an independent reduction recover a mid-transit time from public TESS photometry, and what does the comparison with the published ephemeris actually mean?

What I work on

  • Archive selection and provenance
  • Aperture photometry and detrending
  • Transit fits and timing uncertainty
  • Injection-recovery tests

Current work

The TESS transit-timing project is the first formal research project. It has a frozen selection rule, a synthetic recovery campaign, two real single-transit fits, and a full-sector cross-check.

The two real fits fix the published period. The cross-check reports where the full-sector and single-transit paths disagree rather than hiding the difference.

Methods and standards

  • Archive requests recorded with times, status codes, and digests
  • A fixed quality mask and aperture rule
  • Covariance and injection-recovery checks
  • Comparison with the published ephemeris before any claim

Directions

  • A physical transit model with fitted limb darkening and dilution
  • Red-noise calibration for real timing uncertainties
  • More target-sector pairs from the docket
  • Small-telescope photometry to extend the time baseline

All research areas. Notes and records are in the notes archive and the data and code index.