Data taking gaps and detection efficiencies

This repository is currently under development and it is not ready to use.

Set of notebooks to estimate the period of times where Gaia was not taking data, or the data taken was not used for the different releases, and compute the detection efficiencies as a function of G magnitude and time.

Work based on the "Completeness of the GaiaVerse" (website, github).

Files in repository

• match_observations_detections.ipynb: Using a scanning law, and a time series of individual star measurements, match the observations (predicted by the scanning law) to detections (published measurements).

• gaps_detection_efficiencies.ipynb: Estimate data taking gaps and detection efficiencies as a function of time and magnitude G.