The stellar occultation technique is a unique and reliable method to investigate the size, shape, and environment around Solar System objects. One of the indispensables of this technique is multi-chord observations. Sometimes collecting observational data and equipment details from observers affects prolonged research time. For this reason, we aimed to create a common online platform where the needed data will be collected and analyzed (producing light curves/photometry) on a single center for ongoing campaign observations.
Occultation Portal is a web-based astronomical archive and analysis platform for aiming the fast, efficient, and centralized management of occultation observation campaigns called by the
Lucky Star Project/Paris Observatory/LESIA and
the ACROSS Project. This platform is a scientific initiative conducted in partnership with a
TÜBİTAK National Observatory (Turkey),
Akdeniz University (Turkey),
The Federal University of Technology – Paraná (Brasil), the
Paris Observatory/LESIA Lucky Star Project (France) and the
Observatoire de la Côte d’Azur - Boulevard de l’Observatoire (France).
For detailed information about the Occultation Portal's software design and architecture, you can review the presentation at the
39th ESOP:
PDF -
Video
For academic use, please cite the paper:
Y Kilic, F Braga-Ribas, M Kaplan, O Erece, D Souami, M Dindar, J Desmars, B Sicardy, B E Morgado, M N Shameoni, F L Rommel, A R Gomes-Júnior,
Occultation portal: A web-based platform for data collection and analysis of stellar occultations, Monthly Notices of the Royal Astronomical Society, Volume 515, Issue 1, September 2022, Pages 1346–1357,
https://doi.org/10.1093/mnras/stac1595 |
NASA/ADS.