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SORA: Stellar Occultation Reduction and Analysis

Authors :
A R Gomes-Júnior
B E Morgado
G Benedetti-Rossi
R C Boufleur
F L Rommel
M V Banda-Huarca
Y Kilic
F Braga-Ribas
B Sicardy
Universidade Estadual Paulista (UNESP)
Lab Juterinst e Astron LIneA & INGT e Universo
Univ PSL
Observ Nacl MCTIC
Akdeniz Univ
TUBITAK Natl Observ
Fed Univ Technol Parana UTFPR DAFIS
Source :
Web of Science, Repositório Institucional da UNESP, Universidade Estadual Paulista (UNESP), instacron:UNESP
Publication Year :
2022
Publisher :
arXiv, 2022.

Abstract

The stellar occultation technique provides competitive accuracy in determining the sizes, shapes, astrometry, etc., of the occulting body, comparable to in-situ observations by spacecraft. With the increase in the number of known Solar System objects expected from the LSST, the highly precise astrometric catalogues, such as Gaia, and the improvement of ephemerides, occultations observations will become more common with a higher number of chords in each observation. In the context of the Big Data era, we developed SORA, an open-source python library to reduce and analyse stellar occultation data efficiently. It includes routines from predicting such events up to the determination of Solar System bodies' sizes, shapes, and positions.<br />Comment: 15 pages, 7 figures

Details

Database :
OpenAIRE
Journal :
Web of Science, Repositório Institucional da UNESP, Universidade Estadual Paulista (UNESP), instacron:UNESP
Accession number :
edsair.doi.dedup.....5437a56daf769918b39560a76d43c231
Full Text :
https://doi.org/10.48550/arxiv.2201.01799