Using pyastrometry_cli_main.py

Introduction

The script “pyastrometry_cli_main.py” handles taking an image and plate solveing it to find the current position of the mount.

Invocation

The invocation of autofocus_auto_star.py is:

usage: pyastrometry_cli <operation> [<args>]

The accepted commands are:
   solvepos     Take an image and solve current position
   solveimage <filename>    Solve position of an image file
   sync         Take an image, solve and sync mount
   slewsolve  <ra> <dec>  Slew to position and plate solve and slew until within threshold

Astromentry CLI

positional arguments:
  operation   Operation to perform

optional arguments:
  -h, --help  show this help message and exit

Command Details

solvepos:

Takes an image with the camera and solves it. Drivers can be specified via a astroprofile or command line arguments.

usage: pyastrometry_cli solvepos [<args>]

Solve Parameters

optional arguments:
  -h, --help            show this help message and exit
  --profile PROFILE     Name of astroprofile
  --mount               Name of mount driver
  --camera              Name of camera driver
  --exposure            Exposure time
  --binning             Camera binning
  --solver SOLVER       Solver to use
  --pixelscale PIXELSCALE
                        Pixel scale (arcsec/pixel)
  --downsample DOWNSAMPLE
                        Downsampling
  --outfile OUTFILE     Output JSON file with solution
  --force               Overwrite output file

Valid solvers are:
    astrometryonline
    astrometrylocal
    platesolve2

solveimage:

Solves an existing image.

usage: pyastrometry_cli solveimage <filename> [<args>]

Solve Parameters

optional arguments:
  -h, --help            show this help message and exit
  --profile PROFILE     Name of astro profile
  --solver SOLVER       Solver to use
  --pixelscale PIXELSCALE
                        Pixel scale (arcsec/pixel)
  --downsample DOWNSAMPLE
                        Downsampling
  --outfile OUTFILE     Output JSON file with solution
  --force               Overwrite output file

Valid solvers are:
    astrometryonline
    astrometrylocal
    platesolve2

sync:

Takes an image with the camera and solves it and syncs mount to solution.

usage: pyastrometry_cli sync [<args>]

Solve Parameters

optional arguments:
  -h, --help            show this help message and exit
  --profile PROFILE     Name of astroprofile
  --mount               Name of mount driver
  --camera              Name of camera driver
  --exposure            Exposure time
  --binning             Camera binning
  --solver SOLVER       Solver to use
  --pixelscale PIXELSCALE
                        Pixel scale (arcsec/pixel)
  --downsample DOWNSAMPLE
                        Downsampling
  --outfile OUTFILE     Output JSON file with solution
  --force               Overwrite output file

Valid solvers are:
    astrometryonline
    astrometrylocal
    platesolve2

slewsolve:

Given an RA/DEC position slew to that position and refine slew using plate solving.

usage: pyastrometry_cli slewsolve <ra> <dec> [<args>]

Solve Parameters

optional arguments:
  -h, --help            show this help message and exit
  --profile PROFILE     Name of astroprofile
  --mount               Name of mount driver
  --camera              Name of camera driver
  --exposure            Exposure time
  --binning             Camera binning
  --solver SOLVER       Solver to use
  --pixelscale PIXELSCALE
                        Pixel scale (arcsec/pixel)
  --downsample DOWNSAMPLE
                        Downsampling
  --outfile OUTFILE     Output JSON file with solution
  --force               Overwrite output file

Valid solvers are:
    astrometryonline
    astrometrylocal
    platesolve2

Using an astroprofile

If specified an astroprofile will be used to get camera and mount driver information as well as the pixelscale used for platesolving.