.. SHERLOCK PIPEline documentation master file, created by sphinx-quickstart on Thu Jul 8 08:43:51 2021. You can adapt this file completely to your liking, but it should at least contain the root `toctree` directive. ============================================= Plan Module ============================================= The ``plan`` module in SHERLOCK provides tools for planning follow-up observations of exoplanet candidates. This module helps astronomers determine optimal observation windows and configurations for confirming candidate planets. Overview -------- The plan module offers capabilities for: - Transit event prediction for follow-up observations - Visibility calculations for specific observatories - Weather and seeing condition integration - Prioritization of targets based on scientific criteria - Generation of observation plans and schedules Usage ----- The observation plan module can be run directly from the command line (within the target directory): .. code-block:: bash # Basic usage for planning observations of a specific candidate # Note: Must specify either observatories file OR coordinates python3 -m sherlockpipe.plan --candidate 1 --observatories observatories.csv # Alternative: specify observatory coordinates directly python3 -m sherlockpipe.plan --candidate 1 --lat 28.3 --lon -16.5 --alt 2400 # For example configuration format, see examples/properties/plan.yaml # ``_ # Note: This module requires Bayesian fit results to be present in the target directory # Example observatories.csv file format: # ``_ The input configuration file typically includes: - Target information (coordinates, magnitudes) - Observatory details (location, capabilities) - Observation constraints (airmass, moon separation) - Time period for planning API Reference ------------ .. autosummary:: :toctree: _autosummary :template: custom-module-template.rst :recursive: sherlockpipe.observation_plan sherlockpipe.plan Integration with External Packages --------------------------------- The plan module integrates with astronomical packages for: - Ephemeris calculations - Observatory visibility computations - Atmospheric condition predictions - Telescope scheduling optimization