ASTR 470 Lab 04: Pulsar timing and braking

Lectures 05-06 ยท high-energy data activity

Objectives

Materials and setup

Use Python 3, the supplied pulsar_timing.csv, and the source documentation named below. The supplied record is clearly labeled in data/README.md. Record file hash, row count, columns, units, processing state, and provenance level.

Computed check: R < 1154.3 AU The bound assumes the observed variability is intrinsic and that the Doppler factor is known.

Procedure

  1. Inspect the file and make a schema table before filtering or fitting.
  2. Reproduce the baseline calculation with units and an independent hand-derived formula.
  3. Apply the activity-specific task: calculate characteristic age, dipole field, and rotational energy loss from timing records.
  4. Perform one perturbation or alternative-model test and report the direction of change.
  5. Write a caption that identifies data, transformation, inference, uncertainty, and limitation.

Measurement and analysis record

RecordRequired entry
InputFile, source, release or access date, columns, units, and provenance level.
ModelEquation, parameter values, boundary conditions, and approximation.
UncertaintyStatistical term plus calibration, distance, response, or model sensitivity.
ValidationIndependent recomputation, limiting-case check, and comparison direction.

Deliverables and assessment

Submit code or notebook, provenance manifest, one labeled figure or table, a 700-word methods memo, and a revision note. Full credit requires traceable input, correct units, explicit assumptions, uncertainty treatment, and a specific limitation. Resubmission with a change log is encouraged.

Sources and provenance

Use Crab-like P and Pdot values and compare the timing age with a supplied historical age; explain braking-index limitations. Reference anchor: OpenStax 23.4 Figure 23.16 and NICER documentation.. Level-1 mission facts are listed separately from level-2 literature/object parameters and level-3 teaching records.