AutoWISP

Contents:

  • Installation
    • Requirements
    • Installing the released version
    • What you just installed
    • A ready-made setup for Windows
    • Installing from source
    • Plate solving
    • Gaia archive access
    • Run the tests (optional)
  • Bringing your own data
    • Sort the images by type
    • Decide which calibrations you have
    • Describe the equipment
    • Tell AutoWISP how to read your headers
    • Registering the images
  • Example: processing the test data one command line step at a time
    • Create a temporary directory to work in (remember to delete it at the end) and enter it
    • Download the test data
    • How the images are organized, and what processing produces
    • Adjust test.cfg before you start
    • Perform the calibration for the zero frames
    • Create a master bias by stacking the calibrated zero frames
    • Perform the calibration for the dark frames
    • Create a master dark by stacking the calibrated dark images
    • Perform calibration for flat frames
    • Build a master flat out of the individual calibrated flat frames
    • Perform calibration for object frames
    • Find stars in the calibrated object frames
    • Perform astrometry on DR files
    • Perform PSF/PRF fitting
    • Perform aperture photometry
    • Run fit source extracted PSF map
    • Perform magnitude fitting
    • Create light curves
    • Perform EPD on light curves
    • Generate EPD statistics file for light curves
    • Perform TFA on light curves
    • Generate TFA statistics file for light curves
    • Extract brightness vs time from lightcurves
  • How a setting gets its value
    • Settings belong to the project
    • A value, and when it applies
    • Where the values come from, and what “no value” means
    • Carrying configuration between projects
    • Settings you will not find in your configuration
    • What the values themselves are
    • A note on versions
  • Diagnostics
    • What gets measured
    • Looking at them
    • What the pipeline does with them
  • Choosing the photometric reference
    • Getting there
    • A starting point, not the final standard
    • One reference per group
    • Start at the top, then look
    • What you are shown
    • Watch where it points
    • Recording the choice
  • Looking at the light curves
    • The first plot
    • Comparing what detrending did
    • Plotting other things
    • Overlaying a transit model
    • The figure itself
  • When something goes wrong
    • The error log
    • Picking up after an interrupted run
    • The logs
    • Sending a crash report
    • Keeping the log from growing
  • Configuration Options
  • autowisp package
    • Subpackages
    • Submodules
AutoWISP
  • autowisp package
  • autowisp.browser_interface package
  • autowisp.browser_interface.django_project package
  • View page source

autowisp.browser_interface.django_project package

Submodules

  • autowisp.browser_interface.django_project.asgi module
  • autowisp.browser_interface.django_project.db_config module
    • _ensure_mysql_driver()
    • get_database_url()
    • get_databases()
    • sqlite_fname
    • url_env_var
    • url_fname
  • autowisp.browser_interface.django_project.settings module
    • Class Inheritance Diagram
  • autowisp.browser_interface.django_project.urls module
  • autowisp.browser_interface.django_project.wsgi module
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© Copyright 2018, Kaloyan Penev.

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