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

Autores
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, Romina Paola; Jofré, E.; Seeliger, M.; Henning, T.
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
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.
Fil: Maciejewski, G.. Nicolaus Copernicus University; Polonia
Fil: Dimitrov, D.. Bulgarian Academy Of Sciences; Bulgaria
Fil: Mancini, L.. Max Planck Institute for Astronomy; Alemania. Osservatorio Astrofisico Di Torino; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Southworth, J.. Keele University; Reino Unido
Fil: Ciceri, S.. Max Planck Institute For Astronomy; Alemania
Fil: D'Ago, G.. Istituto Internazionale per gli Alti Studi ; Italia
Fil: Bruni, I.. Osservatorio Astrofisico di Bologna; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Raetz, St.. Universitat Erlangen-nurmberg. Astronomisches Institut-dr. Karl Remeis-sternwarte & Ecap; Alemania. European Space Agency; Países Bajos
Fil: Nowak, G.. Instituto de Astrofísica de Canarias; España. Nicolaus Copernicus University; Polonia. Universidad de La Laguna; España
Fil: Ohlert, J.. University of Applied Sciences; Alemania. Michael Adrian Observatorium; Alemania
Fil: Puchalski, D.. Nicolaus Copernicus University; Polonia
Fil: Saral, G.. Istanbul University; Turquía. University Of Geneva (ug);
Fil: Derman, E.. Ankara University; Turquía
Fil: Petrucci, Romina Paola. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Jofré, E.. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Seeliger, M.. Universitat Erlangen-nurmberg. Astronomisches Institut-dr. Karl Remeis-sternwarte & Ecap; Alemania
Fil: Henning, T.. Max Planck Institute for Astronomy; Alemania
Materia
PLANETARY SYSTEMS
PLANETS AND SATELLITES: INDIVIDUAL: HAT-P-30 b, HAT-P-37 b, TrES- 5 b, WASP-28 b, WASP-36 b, WASP-39 b
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/181017
Acceder
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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling New Transit Observations for HAT-P-30 b, HAT-P-37 b, TrES-5 b, WASP-28 b, WASP-36 b and WASP-39 bMaciejewski, 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, Romina PaolaJofré, E.Seeliger, M.Henning, T.PLANETARY SYSTEMSPLANETS AND SATELLITES: INDIVIDUAL: HAT-P-30 b, HAT-P-37 b, TrES- 5 b, WASP-28 b, WASP-36 b, WASP-39 bhttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1We 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.Fil: Maciejewski, G.. Nicolaus Copernicus University; PoloniaFil: Dimitrov, D.. Bulgarian Academy Of Sciences; BulgariaFil: Mancini, L.. Max Planck Institute for Astronomy; Alemania. Osservatorio Astrofisico Di Torino; Italia. Istituto Nazionale di Astrofisica; ItaliaFil: Southworth, J.. Keele University; Reino UnidoFil: Ciceri, S.. Max Planck Institute For Astronomy; AlemaniaFil: D'Ago, G.. Istituto Internazionale per gli Alti Studi ; ItaliaFil: Bruni, I.. Osservatorio Astrofisico di Bologna; Italia. Istituto Nazionale di Astrofisica; ItaliaFil: Raetz, St.. Universitat Erlangen-nurmberg. Astronomisches Institut-dr. Karl Remeis-sternwarte & Ecap; Alemania. European Space Agency; Países BajosFil: Nowak, G.. Instituto de Astrofísica de Canarias; España. Nicolaus Copernicus University; Polonia. Universidad de La Laguna; EspañaFil: Ohlert, J.. University of Applied Sciences; Alemania. Michael Adrian Observatorium; AlemaniaFil: Puchalski, D.. Nicolaus Copernicus University; PoloniaFil: Saral, G.. Istanbul University; Turquía. University Of Geneva (ug);Fil: Derman, E.. Ankara University; TurquíaFil: Petrucci, Romina Paola. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Jofré, E.. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Seeliger, M.. Universitat Erlangen-nurmberg. Astronomisches Institut-dr. Karl Remeis-sternwarte & Ecap; AlemaniaFil: Henning, T.. Max Planck Institute for Astronomy; AlemaniaCopernicus Foundation Polish Astronomy2016-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/181017Maciejewski, G.; Dimitrov, D.; Mancini, L.; Southworth, J.; Ciceri, S.; et al.; 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; Copernicus Foundation Polish Astronomy; Acta Astronomica; 66; 1-2016; 55-740001-52370001-5237CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://acta.astrouw.edu.pl/Vol66/n1/a_66_1_4.htmlinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1603.03268info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:43:47Zoai:ri.conicet.gov.ar:11336/181017instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:43:47.668CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv 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
title 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
spellingShingle 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
Maciejewski, G.
PLANETARY SYSTEMS
PLANETS AND SATELLITES: INDIVIDUAL: HAT-P-30 b, HAT-P-37 b, TrES- 5 b, WASP-28 b, WASP-36 b, WASP-39 b
title_short 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
title_full 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
title_fullStr 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
title_full_unstemmed 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
title_sort 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
dc.creator.none.fl_str_mv 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, Romina Paola
Jofré, E.
Seeliger, M.
Henning, T.
author Maciejewski, G.
author_facet 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, Romina Paola
Jofré, E.
Seeliger, M.
Henning, T.
author_role author
author2 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, Romina Paola
Jofré, E.
Seeliger, M.
Henning, T.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv PLANETARY SYSTEMS
PLANETS AND SATELLITES: INDIVIDUAL: HAT-P-30 b, HAT-P-37 b, TrES- 5 b, WASP-28 b, WASP-36 b, WASP-39 b
topic PLANETARY SYSTEMS
PLANETS AND SATELLITES: INDIVIDUAL: HAT-P-30 b, HAT-P-37 b, TrES- 5 b, WASP-28 b, WASP-36 b, WASP-39 b
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv 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.
Fil: Maciejewski, G.. Nicolaus Copernicus University; Polonia
Fil: Dimitrov, D.. Bulgarian Academy Of Sciences; Bulgaria
Fil: Mancini, L.. Max Planck Institute for Astronomy; Alemania. Osservatorio Astrofisico Di Torino; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Southworth, J.. Keele University; Reino Unido
Fil: Ciceri, S.. Max Planck Institute For Astronomy; Alemania
Fil: D'Ago, G.. Istituto Internazionale per gli Alti Studi ; Italia
Fil: Bruni, I.. Osservatorio Astrofisico di Bologna; Italia. Istituto Nazionale di Astrofisica; Italia
Fil: Raetz, St.. Universitat Erlangen-nurmberg. Astronomisches Institut-dr. Karl Remeis-sternwarte & Ecap; Alemania. European Space Agency; Países Bajos
Fil: Nowak, G.. Instituto de Astrofísica de Canarias; España. Nicolaus Copernicus University; Polonia. Universidad de La Laguna; España
Fil: Ohlert, J.. University of Applied Sciences; Alemania. Michael Adrian Observatorium; Alemania
Fil: Puchalski, D.. Nicolaus Copernicus University; Polonia
Fil: Saral, G.. Istanbul University; Turquía. University Of Geneva (ug);
Fil: Derman, E.. Ankara University; Turquía
Fil: Petrucci, Romina Paola. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Jofré, E.. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Seeliger, M.. Universitat Erlangen-nurmberg. Astronomisches Institut-dr. Karl Remeis-sternwarte & Ecap; Alemania
Fil: Henning, T.. Max Planck Institute for Astronomy; Alemania
description 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.
publishDate 2016
dc.date.none.fl_str_mv 2016-01
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/181017
Maciejewski, G.; Dimitrov, D.; Mancini, L.; Southworth, J.; Ciceri, S.; et al.; 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; Copernicus Foundation Polish Astronomy; Acta Astronomica; 66; 1-2016; 55-74
0001-5237
0001-5237
CONICET Digital
CONICET
url http://hdl.handle.net/11336/181017
identifier_str_mv Maciejewski, G.; Dimitrov, D.; Mancini, L.; Southworth, J.; Ciceri, S.; et al.; 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; Copernicus Foundation Polish Astronomy; Acta Astronomica; 66; 1-2016; 55-74
0001-5237
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://acta.astrouw.edu.pl/Vol66/n1/a_66_1_4.html
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1603.03268
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv Copernicus Foundation Polish Astronomy
publisher.none.fl_str_mv Copernicus Foundation Polish Astronomy
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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