English

Occultation Portal: a web-based platform for data collection and analysis of stellar occultations

Solar and Stellar Astrophysics 2022-06-22 v1 Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics

Abstract

Recording a stellar occultation is one powerful method that gives direct information about the physical properties of the occulting solar system object. In order to obtain reliable and accurate results, simultaneous observations from different locations across-track of the projected path are of great importance. However, organising all the observing stations, aggregating, and analysing the data is time-consuming and not that easy. We have developed a web portal named Occultation Portal (OP) to manage all those occultation observation campaigns from a central server. With this portal, the instrumental and observational information of all observers participating in a stellar occultation campaign and the concerned data are archived systematically in a standard format. The researchers can then visualise the archived data on an event basis. The investigators can also extract the light curve for each data-set with the added reduction pipeline to the portal base. This paper describes in detail the portal structure and the developed features.

Keywords

Cite

@article{arxiv.2206.09615,
  title  = {Occultation Portal: a web-based platform for data collection and analysis of stellar occultations},
  author = {Y. Kilic and F. Braga-Ribas and M. Kaplan and O. Erece and D. Souami and M. Dindar and J. Desmars and B. Sicardy and B. E. Morgado and M. N. Shameoni and F. L. Rommel and A. R. Gomes-Júnior},
  journal= {arXiv preprint arXiv:2206.09615},
  year   = {2022}
}

Comments

13 pages, 12 figures, 1 table, and 1 listing, accepted for publication in MNRAS