Lab 05: Weak-lensing parameter combinations

ASTR 476: Observational Cosmology · 2026-09-25

Scope: Lectures 09-10 · Purpose: Translate DES Y3 S8 and Omega_m summaries into conditional sigma8 values and quantify how fixed-Omega_m assumptions affect interpretation.

Setup and data

Procedure

  1. Load DES Y3 S8 and Omega_m values and preserve asymmetric bounds.
  2. Invert the S8 definition at the central Omega_m to obtain sigma8.
  3. Evaluate sigma8 across the Omega_m lower and upper endpoints while holding S8 fixed; label this sensitivity, not a confidence interval.
  4. Draw the S8 constant contour and explain the compressed degeneracy direction.
  5. List the missing covariance and nuisance information needed for a proper propagated posterior.

Deliverables

Deliver: calculation, a parameter-space plot, asymmetric endpoint table, and an interpretation separating conditional transformation from posterior inference.

Assessment criteria

Rubric: correct algebra 25%; bounds and assumptions 25%; plot readability 15%; missing-covariance reasoning 25%; provenance 10%.

Uncertainty and interpretation

Report numerical precision, input uncertainty, model assumptions, and covariance availability separately. Label every output as directly measured, published summary, derived, or model/synthetic. A successful script run is not evidence that the scientific interpretation is valid.

Revisions and resubmissions are encouraged. Credit is based on defensible reasoning, validation, provenance, and clear limitations.

ASTR 476 · Lab 05 · paired-module cadence Lectures 09-10 · version 2026-09-25