Optimized cutting off transit algorithm to study stellar rotation from PLATO mission light curves
| Autor: | Leandro de Almeida, Reza Samadi, Francys Anthony, Jefferson Soares da Costa, Ana Carolina Mattiuci, Matthieu Castro, José Dias do Nascimento |
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| Přispěvatelé: | Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP) |
| Jazyk: | angličtina |
| Rok vydání: | 2020 |
| Předmět: |
Brown dwarf
Data analysis FOS: Physical sciences Astrophysics::Cosmology and Extragalactic Astrophysics 01 natural sciences Space exploration Planet 0103 physical sciences Astrophysics::Solar and Stellar Astrophysics Transit (astronomy) Stellar rotation 010303 astronomy & astrophysics Solar and Stellar Astrophysics (astro-ph.SR) Astrophysics::Galaxy Astrophysics Physics [PHYS]Physics [physics] 010308 nuclear & particles physics Astronomy Astronomy and Astrophysics Planetary system Light curve Eclipsing binaries Stars Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science Astrophysics::Earth and Planetary Astrophysics [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
| Zdroj: | Repositório Institucional da UFRN Universidade Federal do Rio Grande do Norte (UFRN) instacron:UFRN Experimental Astronomy Experimental Astronomy, Springer Link, 2020, 50 (1), pp.73-90. ⟨10.1007/s10686-020-09664-x⟩ |
| ISSN: | 0922-6435 1572-9508 |
| DOI: | 10.1007/s10686-020-09664-x⟩ |
| Popis: | Measuring the stellar rotation of one of the components in eclipsing binaries (EBs) or planetary systems is a challenging task. The difficulty is mainly due to the complexity of analyzing, in the same light curve, the signal from the stellar rotation mixed with the transit signal of a stellar or sub-stellar companion, like a brown dwarf or planet. There are many methods to correct the long-term trend of the light curve. However, the correction often erases the signal of the stellar rotation from spots crossing the visible stellar disk and other weaker signals like planets. In this work, we present the DiffeRencial flUx Method of cuTting Off biNariES (DRUM TONES) to identify the signal of the binary transits and disentangle it from stellar rotation planet signals. We present our technique with applications to EBs from CoRoT, Kepler, Kepler K2 and TESS missions. We also applied our method to simulated synthetic EB from the PLATO mission. Our method shows good agreement in the determination of stellar rotation periods for few observed targets from last space missions, as well it is naturally useful for future European missions, such as PLAnetary Transits and Oscillations of stars (PLATO). 21 pages, 10 figures, accepted to be published on The Experimental Astronomy (May 14, 2020) |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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