Open Issues Need Help
View All on GitHubAnything can happen in the next half hour (including spectral timing made easy)!
Anything can happen in the next half hour (including spectral timing made easy)!
Anything can happen in the next half hour (including spectral timing made easy)!
Anything can happen in the next half hour (including spectral timing made easy)!
Anything can happen in the next half hour (including spectral timing made easy)!
Anything can happen in the next half hour (including spectral timing made easy)!
Anything can happen in the next half hour (including spectral timing made easy)!
Anything can happen in the next half hour (including spectral timing made easy)!
Anything can happen in the next half hour (including spectral timing made easy)!
Anything can happen in the next half hour (including spectral timing made easy)!
Anything can happen in the next half hour (including spectral timing made easy)!
AI Summary: The task is to modify the Stingray software package to correctly account for the bin center when calculating times from X-ray data, specifically addressing the `TIMEDEL` and `TIMEPIXR` keywords in the FITS header. This involves understanding the existing time calculation method in Stingray, incorporating the missing keywords into the calculation, and thoroughly testing the changes to ensure accuracy and compatibility with various data formats.
Anything can happen in the next half hour (including spectral timing made easy)!
AI Summary: Update the Stingray Python package to use the correct replacement for the deprecated `jax.interpreters.xla.pytype_aval_mappings` function, resolving a compatibility issue with JAX version 0.7.0 and later. This involves identifying the usage of the deprecated function within the `test_gpmodeling.py` file and replacing it with `jax.core.pytype_aval_mappings`.
Anything can happen in the next half hour (including spectral timing made easy)!
AI Summary: Debug and correct a normalization error in the Stingray software package's power spectral density calculation. The issue lies in the `normalize_abs` function, which is incorrectly calculating the absolute power spectral normalization by a factor of dt^2. The task involves understanding the existing code, identifying the source of the error in the normalization formula, and implementing the necessary correction.
Anything can happen in the next half hour (including spectral timing made easy)!