Occultation portal: A web-based platform for data collection and analysis of stellar occultations

Author:

Kilic Y12,Braga-Ribas F345,Kaplan M1ORCID,Erece O12,Souami D678ORCID,Dindar M2,Desmars J910,Sicardy B7,Morgado B E45711ORCID,Shameoni M N12,Rommel F L45,Gomes-Júnior A R513ORCID

Affiliation:

1. Department of Space Sciences and Technologies, Akdeniz University , Campus, Antalya 07058, Turkey

2. TÜBİTAK National Observatory, Akdeniz University Campus , Antalya 07058, Turkey

3. Federal University of Technology, Parana (UTFPR-Curitiba) , Curitiba, PR 81280-340, Brazil

4. Observatório Nacional/MCTIC , R. General José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil

5. Laboratório Interinstitucional de e-Astronomia - LIneA and INCT do e-Universo , Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil

6. Université Côte d’Azur, Observatoire de la Côte d’Azur , CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, F-06304 Nice Cedex 4, France

7. LESIA, Observatoire de Paris, Université PSL , CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, F-92195 Meudon, France

8. naXys, University of Namur , 8 Rempart de la Vierge, B-5000 Namur, Belgium

9. Institut Polytechnique des Sciences Avancées IPSA , 63 boulevard de Brandebourg, F-94200 Ivry-sur-Seine, France

10. Institut de Mécanique Céleste et de Calcul des Éphémérides, IMCCE, Observatoire de Paris, PSL Research University, CNRS,Sorbonne Universités , UPMC Univ Paris 06, Univ. Lille, 77 Av. Denfert-Rochereau, F-75014 Paris, France

11. Universidade Federal do Rio de Janeiro - Observatório do Valongo ,Ladeira Pedro Antônio 43, CEP 20080-090, Rio de Janeiro, RJ, Brazil

12. Atatürk University Application and Research Center for Astrophysics (ATASAM) , 25240 Erzurum, Turkey

13. UNESP, São Paulo State University , Grupo de Dinâmica Orbital e Planetologia, CEP 12516-410, Guaratinguetá, SP 12516-410, Brazil

Abstract

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, organizing 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 visualize 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.

Funder

Akdeniz University

European Research Council

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior

CNPq

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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