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1SWASP J200503.05-343726.5: A high mass ratio eclipsing binary near the period limit
Institution:1. Yunnan Observatories, Chinese Academy of Sciences, P.O. Box 110, Kunming 650216, PR China;2. Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, PR China;3. Graduate University of Chinese Academy of Sciences, Beijing, PR China;4. Department of Theoretical Physics and Astrophysics, Masaryk University, Kotlár?ská 2, Brno 611 37, Czech Republic;1. Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, H-1121 Budapest, Konkoly Thege Miklós út 15-17, Hungary;2. BSObservatory, Modrá 587, Zlín 760 01, Czech Republic;1. Department of Astronomy and Astrophysics, Tata Institute of Fundamental Research, Mumbai 400005, India;2. Dipartimento di Fisica, Università di Pisa, Largo B. Pontecorvo, 3 I-56127 Pisa, Italy;3. INFN, Sezione di Pisa, Largo B. Pontecorvo, 3 I-56127 Pisa, Italy;4. Astroparticle Physics and Cosmology Division, Saha Institute of Nuclear Physics, HBNI, 1 / AF Bidhannagar, Kolkata-700064, India;5. Department of Physics, St. Joseph’s College, 36 Lalbagh Road, Bangalore 560027, India;6. Inter-University Centre for Astronomy and Astrophysics (IUCAA), Post Bag 4, Ganeshkhind, Savitribai Phule Pune University, Campus, Pune 411007, India;1. Astrophysical Sciences Division, Bhabha Atomic Research Center, Mumbai 400 085, India;2. Department of High Energy Physics, Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400 005, India;1. Istituto per l''Ambiente Marino Costiero, Consiglio Nazionale delle Ricerche, Calata Porta di Massa, Porto di Napoli, I-80133 Naples, Italy;2. Dipartimento di Scienze — Sezione Geologia, Università degli Studi Roma Tre, Largo San Leonardo Murialdo, 1, I-00146 Rome, Italy;3. Istituto di Geologia Ambientale e Geoingegneria (IGAG-CNR), Area della Ricerca Roma 1 Montelibretti, Via Salaria, Monterotondo Scalo, I-00016 Rome, Italy
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