New Transit Observations for HAT-P-30 b, HAT-P-37 b, TrES-5 b, WASP-28 b, WASP-36 b and WASP-39 b

• Autorzy: Maciejewski, G. , Dimitrov, D. , Mancini, L. , Southworth, J. , Ciceri, S. , D'Ago, G. , Bruni, I. , Raetz, St. , Nowak, G. , Ohlert, J. , Puchalski, D. , Saral, G. , Derman, E. , Petrucci, R. , Jofre, E. , Seeliger, M. , Henning, T.
• Języki publikacji: EN

Abstrakty

EN

We present new transit light curves for planets in six extrasolar planetary systems. They were acquired with 0.4-2.2 m telescopes located in west Asia, Europe, and South America. When combined with literature data, they allowed us to redetermine system parameters in a homogeneous way. Our results for individual systems are in agreement with values reported in previous studies. We refined transit ephemerides and reduced uncertainties of orbital periods by a factor between 2 and 7. No sign of any variations in transit times was detected for the planets studied.

Słowa kluczowe

EN

HAT-P-30 b; HAT-P-37 b; TrES-5 b; WASP-28 b; WASP-36 b; WASP-39 b

• Czasopismo: Acta Astronomica
• Rocznik: 2016
• Tom: Vol. 66, No. 1
• Strony: 55--74
• Opis fizyczny: Bibliogr. 33 poz., rys., tab.

Twórcy

autor

Maciejewski, G.

• Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziądzka 5, 87-100 Toruń, Poland,

autor

Dimitrov, D.

• Institute of Astronomy, Bulgarian Academy of Sciences, 72 Tsarigradsko Chausse Blvd., 1784 Sofia, Bulgaria

autor

Mancini, L.

• Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
• INAF - Osservatorio Astrofisico di Torino, via Osservatorio 20, 10025 - Pino Torinese, Italy

autor

Southworth, J.

• Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK

autor

Ciceri, S.

• Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany

autor

D'Ago, G.

• Istituto Internazionale per gli Alti Studi Scientifici (IIASS), 84019 Vietri Sul Mare, Italy

autor

Bruni, I.

• INAF - Osservatorio Astrofisico di Bologna, via Ranzani 1, 40127 Bologna, Italy

autor

Raetz, St.

• Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergässchen 2-3, 07745 Jena, Germany
• European Space Agency, ESTEC, SRE-S, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands

autor

Nowak, G.

• Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziądzka 5, 87-100 Toruń, Poland
• Instituto de Astrofisica de Canarias, C/ via Lactea, s/n, E-38205 La Laguna, Tenerife, Spain
• Departamento de Astrofisica, Universidad de La Laguna, Av. Astrofisico Francisco Sanchez, s/n, E-38206 La Laguna, Tenerife, Spain

autor

Ohlert, J.

• Michael Adrian Observatorium, Astronomie Stiftung Trebur, 65468 Trebur, Germany
• University of Applied Sciences, Technische Hochschule Mittelhessen, 61169 Friedberg, Germany

autor

Puchalski, D.

• Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziądzka 5, 87-100 Toruń, Poland,

autor

Saral, G.

• University of Geneva, Department of Astronomy, Ch. d'Ecogia 16, 1290 Versoix, Switzerland
• Istanbul University, Graduate School of Science and Engineering, Bozdogan Kemeri Cad. 8, Vezneciler-Istanbul, Turkey

autor

Derman, E.

• Astronomy and Space Sciences Department, Ankara University, 06100 Tandogan, Ankara, Turkey

autor

Petrucci, R.

• Observatorio Astronomico de Cordoba, Laprida 854, X5000 BGR Cordoba, Argentina
• Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Argentina

autor

Jofre, E.

• Observatorio Astronomico de Cordoba, Laprida 854, X5000 BGR Cordoba, Argentina
• Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Argentina

autor

Seeliger, M.

• Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergässchen 2-3, 07745 Jena, Germany

autor

Henning, T.

• Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany

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Uwagi

Opracowanie rekordu w ramach umowy 509/P-DUN/2018 ze środków MNiSW przeznaczonych na działalność upowszechniającą naukę (2019).