1. Shot noise at 100 s 20 points
Compute the photon shot noise (in electrons) for the V=18 worked-scenario star (count rate 243408.201 e⁻/s) after a 100 s exposure.
Problem set for lecture unit 3.
Compute the photon shot noise (in electrons) for the V=18 worked-scenario star (count rate 243408.201 e⁻/s) after a 100 s exposure.
Compare your Problem 1 result to the representative read noise (3.5 e⁻) and dark-current shot noise (0.3162 e⁻ at 100 s), and identify which of the three terms dominates the total noise at this exposure time.
Solve for the exposure time at which shot noise from this source equals the 3.5-electron read-noise floor, and confirm your answer against 0.0 s.
Explain what regime (read-noise-limited or shot-noise-limited) applies for exposures shorter than your Problem 3 answer, and what regime applies for longer exposures, and state which regime is more efficient to operate in for a faint, read-noise-sensitive measurement.
Submit a complete derivation with equations, units, labeled quantities, and a short narrative interpretation for each problem. Show every step; a correct final number without a visible derivation receives partial credit at most, and quoting a lecture number without adapting it to this problem's specific inputs receives no credit for that step.
OpenStax Astronomy 2e (local reference copy: references/openstax-astronomy-2e-extracted.txt), Chapter 6 (astronomical instruments), descriptive only; this course exceeds that introductory treatment throughout.
materials/ASTR340/data/ where referenced above.