Dataciencia

Colección SciELO Chile

HATS-1b: The first transiting planet discovered by the hatsouth survey

Indexado

WoS	WOS:000312251100005
Scopus	SCOPUS_ID:84870178699

DOI

10.1088/0004-6256/145/1/5

Año

2013

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

We report the discovery of HATS-1b, a transiting extrasolar planet orbiting the moderately bright V = 12.05 G dwarf star GSC 6652-00186, and the first planet discovered by HATSouth, a global network of autonomous wide-field telescopes. HATS-1b has a period of P approximate to 3.4465 days, mass of M-p approximate to 1.86 M-J, and radius of R-p approximate to 1.30 R-J. The host star has a mass of 0.99 M-circle dot and radius of 1.04 R-circle dot. The discovery light curve of HATS-1b has near-continuous coverage over several multi-day timespans, demonstrating the power of using a global network of telescopes to discover transiting planets.

Revista

Revista	ISSN
Astronomical Journal	0004-6256

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Penev, Kaloyan	Hombre	Princeton Univ - Estados Unidos Harvard Smithsonian Ctr Astrophys - Estados Unidos Princeton University - Estados Unidos Harvard-Smithsonian Center for Astrophysics - Estados Unidos
2	Bakos, Gaspar	Hombre	Princeton Univ - Estados Unidos Harvard Smithsonian Ctr Astrophys - Estados Unidos Princeton University - Estados Unidos Harvard-Smithsonian Center for Astrophysics - Estados Unidos
3	Bayliss, Dan	Hombre	Australian Natl Univ - Australia Australian National University - Australia The Australian National University - Australia
4	JORDAN-COLZANI, ANDRES CRISTOBAL	Hombre	Pontificia Universidad Católica de Chile - Chile Centro de Excelencia en Astrofísica y Tecnologías Afines - Chile
6	Zhou, George	Hombre	Australian Natl Univ - Australia Australian National University - Australia The Australian National University - Australia
7	Suc, Vincent	Hombre	Pontificia Universidad Católica de Chile - Chile
8	Rabus, M.	Hombre	Pontificia Universidad Católica de Chile - Chile
9	Hartman, Joel D.	Hombre	Princeton Univ - Estados Unidos Harvard Smithsonian Ctr Astrophys - Estados Unidos Princeton University - Estados Unidos Harvard-Smithsonian Center for Astrophysics - Estados Unidos
10	Mancin, L.	Hombre	Max Planck Inst Astron - Alemania Max Planck Institute for Astronomy - Alemania
11	Béky, B.	-	Harvard Smithsonian Ctr Astrophys - Estados Unidos
12	Csubry, Z.	-	Princeton Univ - Estados Unidos Harvard Smithsonian Ctr Astrophys - Estados Unidos Princeton University - Estados Unidos Harvard-Smithsonian Center for Astrophysics - Estados Unidos
13	Buchhave, L. A.	Hombre	Univ Copenhagen - Dinamarca Niels Bohr Institute - Dinamarca Niels Bohr Institutet - Dinamarca
14	Henning, Thomas	Hombre	Max Planck Inst Astron - Alemania Max Planck Institute for Astronomy - Alemania
15	Nikolov, Nikolay	Hombre	Max Planck Inst Astron - Alemania Max Planck Institute for Astronomy - Alemania
16	Csák, B.	-	Max Planck Inst Astron - Alemania
17	BRAHM-SCOTT, RAFAEL ANDRES	Hombre	Pontificia Universidad Católica de Chile - Chile
18	Espinoza, Nestor	Hombre	Pontificia Universidad Católica de Chile - Chile
19	Conroy, P.	-	Australian Natl Univ - Australia Australian National University - Australia The Australian National University - Australia
20	Noyes, R. W.	-	Harvard Smithsonian Ctr Astrophys - Estados Unidos
21	Sasselov, Dimitar	Hombre	Harvard Smithsonian Ctr Astrophys - Estados Unidos Harvard-Smithsonian Center for Astrophysics - Estados Unidos
22	Schmidt, Brian	Hombre	Australian Natl Univ - Australia Australian National University - Australia The Australian National University - Australia
23	Wright, Duncan	Hombre	Univ New S Wales - Australia University of New South Wales (UNSW) Australia - Australia UNSW Sydney - Australia
24	Tinney, C. G.	Hombre	Univ New S Wales - Australia University of New South Wales (UNSW) Australia - Australia UNSW Sydney - Australia
25	Addison, B.	Hombre	Univ New S Wales - Australia University of New South Wales (UNSW) Australia - Australia UNSW Sydney - Australia
26	Lazar, J.	-	Hungarian Astron Assoc - Hungría
27	Papp, I.	-	Hungarian Astron Assoc - Hungría
28	Mohler, M.	-	Max Planck Inst Astron - Alemania
28	Sari, P.	-	Hungarian Astron Assoc - Hungría

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Origen de Citas Identificadas

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 58.18 %
Citas No-identificadas: 41.82 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

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Citas No-identificadas: 41.82 %

Financiamiento

Fuente
Anillo
Robert Martin Ayers Sciences Fund
Fondecyt Project
NSF MRI grant
NASA grant
SIMBAD database
ARC Laureate Fellowship Grant
BASAL CATA PFB-06
ALMA-CONICYT FUND Project
Ministry of Economy ICM Nuclei
FEROS ID programmes
Fondencyt postdoctoral fellowship
GROND ID programme
ESO at the La Silla Observatory
Directorate for Mathematical and Physical Sciences

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Agradecimientos

Agradecimiento
Development of the HATSouth project was funded by NSF MRI grant NSF/AST-0723074, operations are supported by NASA grant NNX09AB29G, and follow-up observations received partial support from grant NSF/AST-1108686. Follow-up observations with the ESO 2.2 m/FEROS instrument were performed under MPI guaranteed time (P087.A-9014(A), P088.A-9008(A), P089.A-9008(A)) and Chilean time (P087.C-0508(A)). A.J. acknowledges support from Fondecyt project 1095213, Ministry of Economy ICM Nuclei P07-021-F and P10-022-F, Anillo ACT-086 and BASAL CATA PFB-06. V. S. acknowledges support form BASAL CATA PFB-06. M. R. acknowledges support from a Fondencyt postdoctoral fellowship N 3120097 and contributions from the ALMA-CONICYT FUND Project N 31090015. R. B. and N. E. acknowledge support from Fondecyt project 1095213. This work is based on observations made with ESO Telescopes at the La Silla Observatory under programme IDs P087.A-9014(A), P088.A-9008(A), P089.A-9008(A), P087.C-0508(A), 089.A-9006(A), and observations made with the Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. This paper also uses observations obtained with facilities of the Las Cumbres Observatory Global Telescope. Work at the Australian National University is supported by ARC Laureate Fellowship Grant FL0992131. We acknowledge the use of the AAVSO Photometric All-Sky Survey (APASS), funded by the Robert Martin Ayers Sciences Fund, and the SIMBAD database, operated at CDS, Strasbourg, France. M. M. thanks N. Piskunov and his group in Uppsala for introducing her to Spectroscopy Made Easy (SME). Operations at the MPG/ESO 2.2 m Telescope are jointly performed by the Max Planck Gesellschaft and the European Southern Observatory. The imaging system GROND has been built by the high-energy group of MPE in collaboration with the LSW Tautenburg and ESO. We thank Timo Anguita and Regis Lachaume for their technical assistance during the observations at the MPG/ESO 2.2 m Telescope. We thank Miguel Roth, Francesco Di Mille, and Rodolfo Angeloni for allowing us to use the Swope telescope on 2011 May 24-25.

Agradecimiento

Development of the HATSouth project was funded by NSF MRI grant NSF/AST-0723074, operations are supported by NASA grant NNX09AB29G, and follow-up observations received partial support from grant NSF/AST-1108686. Follow-up observations with the ESO 2.2 m/FEROS instrument were performed under MPI guaranteed time (P087.A-9014(A), P088.A-9008(A), P089.A-9008(A)) and Chilean time (P087.C-0508(A)). A.J. acknowledges support from Fondecyt project 1095213, Ministry of Economy ICM Nuclei P07-021-F and P10-022-F, Anillo ACT-086 and BASAL CATA PFB-06. V. S. acknowledges support form BASAL CATA PFB-06. M. R. acknowledges support from a Fondencyt postdoctoral fellowship N 3120097 and contributions from the ALMA-CONICYT FUND Project N 31090015. R. B. and N. E. acknowledge support from Fondecyt project 1095213. This work is based on observations made with ESO Telescopes at the La Silla Observatory under programme IDs P087.A-9014(A), P088.A-9008(A), P089.A-9008(A), P087.C-0508(A), 089.A-9006(A), and observations made with the Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. This paper also uses observations obtained with facilities of the Las Cumbres Observatory Global Telescope. Work at the Australian National University is supported by ARC Laureate Fellowship Grant FL0992131. We acknowledge the use of the AAVSO Photometric All-Sky Survey (APASS), funded by the Robert Martin Ayers Sciences Fund, and the SIMBAD database, operated at CDS, Strasbourg, France. M. M. thanks N. Piskunov and his group in Uppsala for introducing her to Spectroscopy Made Easy (SME). Operations at the MPG/ESO 2.2 m Telescope are jointly performed by the Max Planck Gesellschaft and the European Southern Observatory. The imaging system GROND has been built by the high-energy group of MPE in collaboration with the LSW Tautenburg and ESO. We thank Timo Anguita and Regis Lachaume for their technical assistance during the observations at the MPG/ESO 2.2 m Telescope. We thank Miguel Roth, Francesco Di Mille, and Rodolfo Angeloni for allowing us to use the Swope telescope on 2011 May 24-25.

Muestra la fuente de financiamiento declarada en la publicación.

Abstract

Revista

Métricas Externas

Disciplinas de Investigación

Colaboración Institucional

Autores - Afiliación

Origen de Citas Identificadas

Financiamiento

Agradecimientos

Departamento Gestión de Conocimiento, Monitoreo y Prospección