Pipeline

Usage

The reason to use the pipeline is for automatic data reduction, finding comparison stars, multi-aperture photometry, etc.

To run the pipeline, simply run:

EB_pipeline -h

This will output the options available to a user for inputs that are allowed or required.

Inputs

There are two required inputs by the user and the first is an input folder. This is the folder pathway where the images that being taken by a telescope are going to. The second required input is the output folder. This is where the user wants the new reudced images and created files to go to.

These next few inputs all have default options and are not required by the user to replace them with.

  • --time How long should the program wait to see if no new files enter the folder and to start the data reduction. The default value is set at 3600 seconds (i.e. 1 hour).

  • --loc Location where the images are being taken. At this point in time, the only allowed locations are BSUO or any site that is in this Astropy list.

  • --ra and --dec These are the right ascension and declination of a target system, respectively. The default values are both set at 00:00:00, so we recommend setting these values.

  • --name Variable is designated for the object, that the user is looking at, name. The default value for this is simply target.

Example

An example script setup for the pipeline would be like the following:

EB_pipeline C:/folder1/folder2/raw_images C:/folder1/folder2/reduced_images --time 3000 --loc CTIO --ra 00:28:27.96 --dec 78:57:42.65 --name NSVS_254037

If the declination of the object is negative then that becomes --dec -78:57:42.65.

Notice the first two values entered for the input folder and output folder do not have any --[name]. The order is also extremely important, as the raw images folder is first and the reduced images folder is second.