ASTR 472 Problem Set 06: Pulsar Dispersion, Timing, and Survey Selection

Student assignment · due date set by instructor

Objectives and instructions

Submit complete derivations, units, assumptions, and a short physical interpretation. Include reproducible code for multi-step calculations and show intermediate values. Cite any external catalog or data product with its release/version. Collaboration on methods is allowed; submitted derivations and prose must be your own. Corrections and resubmissions with a change log are encouraged.

Problems

Problem 1: Cold-plasma delay (30 points)

For DM=56.8 pc cm^-3, compute delay between 400 and 1400 MHz. If DM uncertainty is 0.2 pc cm^-3, propagate its contribution to delay uncertainty.

Required: derivation, units, intermediate values, uncertainty/assumption, and an interpretation that identifies what the result does not prove.

Problem 2: Timing and channel smearing (30 points)

A 400-MHz observation uses 0.1-MHz channels and DM=56.8. Estimate intra-channel dispersive smearing from the derivative of the delay law. Compare with a 2-ms pulse width and state the detectability consequence.

Required: derivation, units, intermediate values, uncertainty/assumption, and an interpretation that identifies what the result does not prove.

Problem 3: Completeness estimate (30 points)

For 84 recovered injections out of 100, compute completeness and binomial standard error. Explain why this does not include sky-position or pulse-width model uncertainty.

Required: derivation, units, intermediate values, uncertainty/assumption, and an interpretation that identifies what the result does not prove.

Reading and data

OpenStax Astronomy 2e §23.4 and Chapter 23 Figuring for Yourself 42-43 (pulsar rotation speed) and 53 (pulse count); ATNF Pulsar Catalogue definitions include P0, P1, and DM.

The numbered anchors were checked against the local OpenStax Astronomy 2e extraction; exercise numbers/page breaks can vary by edition. Before assigning through an LMS, the instructor should spot-check each recommendation against the adopted print/PDF edition. Exact source scope and extraction notes are in ../reference-log.md. Do not present the synthetic teaching records as telescope observations.

Deliverables and scoring

Three problems, 100 points total. Submit a PDF or HTML report plus code/notebook where requested. Show figures with axes, units, captions, and data provenance.