Suggested 14-Week Course Schedule#
This is a reading and project sequence designed around a single semester. The course can be compressed or expanded, but Chapters A Guided Tour: What Does a Telescope Actually Record, and Where Is This Book Taking You?–Correlators and Event-Table Data Analysis are best kept intact; all of the later science cases depend on the language of event tables, coherence functions, instrumental errors, and correlators.
Course Goals and Grading Structure#
By the end of the course, students should be able to start from a science question and write down the observable, the event-table fields, the core formulas, the order of magnitude, the error budget, the null tests, and reproducible code. A suggested grading structure is: weekly reading notes \(20\%\), three short computational assignments \(30\%\), one midterm project design \(20\%\), and a final project report and code \(30\%\).
Deliverable |
Content |
Evaluation criteria |
|---|---|---|
Reading notes |
1 page per week, listing the main observables, formulas, orders of magnitude, and open questions. |
Whether the conditions of validity of the formulas are understood, not substituting copied summaries for understanding. |
Short assignments |
Event tables, \(g^{(2)}\), visibility, Fisher information, or error budgets. |
Correct units, clear figures, runnable code. |
Midterm design |
An executable observing or experimental plan. |
Whether the photon rate, baseline, background, calibration, and failure criteria are complete. |
Final project |
Code, PDF figures, a short report, and null tests. |
Whether it can be reproduced, whether systematic errors are explained. |
Weeks 1–5: Foundations and Instruments#
Week |
Reading |
Class focus |
Assignment |
|---|---|---|---|
1 |
Chapter A Guided Tour: What Does a Telescope Actually Record, and Where Is This Book Taking You? |
Event tables, observables, units, and orders of magnitude. |
From the same event table, generate a light curve and one simple statistic. |
2 |
Chapters A Guided Tour: What Does a Telescope Actually Record, and Where Is This Book Taking You?–Single-Mode States of Light: Number, Coherent, Thermal, and Squeezed States |
Why the mean intensity is not enough; common light states. |
Compare the count statistics of thermal light and coherent light. |
3 |
Chapter The Coherence Functions g^{(1)}, g^{(2)} and the Siegert Relation |
\(g^{(1)}\), \(g^{(2)}\), the Siegert relation, and multimode dilution. |
Plot the \(g^{(2)}\) contrast for different mode numbers and time bins. |
4 |
Chapter Spatial Coherence, van Cittert–Zernike, and Intensity Interferometry |
VCZ, uniform disk, binary stars, and intensity-interferometry SNR. |
Fit the angular diameter of a simulated uniform disk. |
5 |
Chapters Detectors, Clocks, and Event Tables–Correlators and Event-Table Data Analysis |
Detectors, time synchronization, correlators, and null tests. |
Write an event-table correlator and complete a time-shift check. |
Weeks 6–10: Source Models and Science Questions#
Week |
Reading |
Class focus |
Assignment |
|---|---|---|---|
6 |
Chapter Quantum Estimation, the Rayleigh Limit, and SPADE Sub-Rayleigh Resolution |
Rayleigh curse, SPADE, and Fisher information. |
Compare the small-separation error of direct imaging versus mode measurement. |
7 |
Chapters The Quantum Language of Astrophysical Radiation Mechanisms–Stars as Quantum Light Sources |
Radiation mechanisms, the thermal-light approximation, stellar angular diameters, and binaries. |
Use $ |
8 |
Chapters White Dwarfs, Neutron Stars, and Strong-Field Physics–Black Holes, Accretion Disks, and the Photon Ring |
Compact objects, pulsars, black holes, and the photon ring. |
Design an event table that preserves phase or time tags. |
9 |
Chapter Bursts, Transients, and Multi-Messenger Quantum Astronomy |
Transient triggers, angular expansion, and multi-messenger delays. |
Build a Type Ia or nova angular-expansion toy model. |
10 |
Chapters Propagation Effects: Plasma, Dust, and Gravitational Lensing–Quantum Problems in Cosmology |
Propagation, polarization rotation, lensing, new physics, and the CMB. |
Distinguish an ordinary propagation term from a new-physics candidate. |
Weeks 11–14: Design, Project, and Report#
Week |
Reading |
Class focus |
Assignment |
|---|---|---|---|
11 |
Chapters Quantum-Network Telescopes–Observation Design, Error Budget, and Feasibility |
Quantum-network boundaries, observing design, and error budgets. |
Write a one-page observing-proposal abstract. |
12 |
Ranking of first-generation science cases. |
Assign readiness scores to three candidate projects. |
|
13 |
Chapters Teaching Experiments and Computational Experiments–Common Misconceptions |
Teaching experiments, common pitfalls, false alarms, and new-physics boundaries. |
Complete the project code, figures, and two null tests. |
14 |
From a textbook project to a proposal. |
Submit the final report, code, and milestone table. |
Final Project Topic Bank#
Topic |
Basic content |
Suggested extension |
|---|---|---|
Tabletop HBT |
Event table, delay histogram, time-shift, response kernel. |
Compare laser, LED, and pseudothermal light. |
Uniform-disk fit |
$ |
V |
Binary intensity interferometry |
Flux ratio, angular separation, position angle, and multi-baseline degeneracy. |
Add orbital phase and mirror degeneracy. |
SPADE toy model |
Mode probabilities, Fisher information, crosstalk, and background. |
Compare different PSFs or centroid errors. |
Type Ia distance |
Angular radius, velocity, explosion time, and distance posterior. |
Add asphericity or a velocity gradient. |
False-alarm analysis |
Poisson tails, trial factor, global significance. |
Use a real or simulated search grid. |