This software enables the creation and management of calibrations that do not require explicit coordinates. It simplifies the calibration process by eliminating the need for coordinate-based systems, improving accuracy and precision, and increasing productivity.
Astro::Coords::Calibration is a Perl module ideally suited for astronomical observations that do not possess any associated coordinates. The module facilitates the creation of a new Astro::Coords::Calibration object with the command: $c = new Astro::Coords::Calibration();
Often, certain observations, such as DARKs and ARRAY TESTS require no specific location of the telescope. This means that they do not have associated coordinates. However, such observations need to be processed in a similar manner as observations with associated coordinates.
This class is an ideal solution for handling such observations. It provides a mechanism to process calibration observations similar to other observations. From a scheduling perspective, calibration observations are always available as a target.
The Astro::Coords::Calibration module is a must-have for those dealing with astronomical observations that do not have associated coordinates. Its implementation aids in processing data related to DARKs and ARRAY TESTS and allows these observations to be handled similar to other observations.
Often, certain observations, such as DARKs and ARRAY TESTS require no specific location of the telescope. This means that they do not have associated coordinates. However, such observations need to be processed in a similar manner as observations with associated coordinates.
This class is an ideal solution for handling such observations. It provides a mechanism to process calibration observations similar to other observations. From a scheduling perspective, calibration observations are always available as a target.
The Astro::Coords::Calibration module is a must-have for those dealing with astronomical observations that do not have associated coordinates. Its implementation aids in processing data related to DARKs and ARRAY TESTS and allows these observations to be handled similar to other observations.
What's New
Version 0.10: N/A