01/2022 by Marc Rosanes-Siscart
Licensed under GNU General Public License V3 (GPLv3) or any later version (GPLv3+)
astrojupyter has been developed during the group practical work of the Master of Astronomy & Astrophysics at VIU (Valencia International University)
This practical work was composed by:
- Observations and Data Acquisition in the OSN (Observatorio de Sierra Nevada, Andalusia): our objective was to observe the primary & secondary transit of WASP-33b and the raw pulsations of its star WASP-33. Data has been acquired for the WASP-33 raw pulsations (evening of 15/11/2021) and the primary transit of WASP-33b (single night from 16-17/11/2021). The secondary transit could not be acquired due to bad weather conditions during the rest of the nights assigned in the OSN for this project.
- Data Analysis of the acquired data: preprocessing with image reduction, normalization, and differential photometry, and postprocessing with the analysis of the obtained light curves.
This project contains some Python Jupyter-Notebooks related to the postprocessing of the light curves obtained with the differential photometry.