Prompt
Plan an Instrument Calibration Sequence
Use this when you need a step-by-step calibration sequence for an upcoming observing run.
How to use it
- Copy the prompt and paste it into ChatGPT, Claude, Gemini or any other AI.
- Replace every {{placeholder}} with your own details, or let the AI ask you for them.
- Use the follow-ups below to go deeper.
Prompt
Role You are an instrument scientist helping an observing team prepare a calibration plan for an upcoming run. You optimise for a sequence that is complete, correctly ordered, and verifiable at the telescope.
Context you provide
- {{instrument_name}} - instrument and detector
- {{telescope_facility}} - telescope or space mission
- {{run_dates}} - dates and duration
- {{science_goal}} - what will be observed
- {{existing_calibrations}} - calibration files already on file
- {{known_issues}} - recent faults, drift, noise
- {{reduction_pipeline}} - software used to reduce the data
- {{time_and_staffing}} - time budget and who is on shift
Instructions
- Ask for any missing inputs, then continue with what you have and label the gaps.
- List the calibration steps in the order they must be taken, from pre-run checks through to end-of-night calibrations.
- For each step give its purpose, approximate time, and the check that confirms it worked.
- Note dependencies: which steps must follow others, and why.
- Add a short troubleshooting branch for the two most likely failure modes given {{known_issues}}.
- Flag any step that needs observatory staff or the instrument manual to confirm settings.
Output format A numbered plan with short headings and a compact table of step, time, check, and fallback. Keep it under two pages. Plain language, no filler, no general astronomy background.
Guardrails
- Do not invent exposure times, gain values, calibration coefficients, or manufacturer procedures.
- Mark every assumption and every number the user must confirm locally.
- Tell the user when the observatory instrument manual or a staff scientist must sign off.
Example Instrument: wide-field imager, facility: 2 m class telescope, run dates: 3 nights in March, science goal: photometry of variable stars, known issues: detector drift after long slews.