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The discovery of the T8.5 dwarf UGPS J0521+3640
Indexado
WoS WOS:000292141600019
DOI 10.1111/J.1745-3933.2011.01062.X
Año 2011
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



We have carried out a search for late-type T dwarfs in the UKIRT Infrared Deep Sky Survey Galactic Plane Survey 6th Data Release. The search yielded two persuasive candidates, both of which have been confirmed as T dwarfs. The brightest, UGPS J0521+3640, has been assigned the spectral type T8.5 and appears to lie at a distance of 7-9 pc. The fainter of the two, UGPS J0652+0324, is classified as a T5.5 dwarf and lies at an estimated distance of 28-37 pc. Warm-Spitzer observations in IRAC channels 1 and 2, taken as part of the GLIMPSE360 Legacy Survey, are available for UGPS J0521+3640 and we used these data with the near-infrared spectroscopy to estimate its properties. We find best-fitting solar metallicity BT-Settl models for T-eff = 600 and 650 K and log g = 4.5 and 5.0. These parameters suggest a mass between 14 and 32M(J) for an age between 1 and 5 Gyr. The proximity of this very cool T dwarf, and its location in the Galactic plane, makes it an ideal candidate for high-resolution adaptive optics imaging to search for cool companions.

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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 Burningham, B. Hombre Univ Hertfordshire - Reino Unido
2 Lucas, Philip Hombre Univ Hertfordshire - Reino Unido
3 Leggett, S. K. - Observatorio Gemini - Estados Unidos
4 Smart, R. L. Hombre Osserv Astron Torino - Italia
5 Baker, D. - Univ Hertfordshire - Reino Unido
6 Pinfield, David J. Hombre Univ Hertfordshire - Reino Unido
7 Tinney, C. G. Hombre Univ New S Wales - Australia
8 Homeier, D. Hombre UNIV GOTTINGEN - Alemania
9 Allard, F. Mujer Ecole Normale Super - Francia
10 Zhang, Z. H. - Univ Hertfordshire - Reino Unido
11 Manatakis, Dimitrios K. Hombre Univ Hertfordshire - Reino Unido
12 DAY-JONES, AVRIL CARA Mujer Universidad de Chile - Chile
13 Jones, Hugh R. A. Hombre Univ Hertfordshire - Reino Unido
14 Kovacs, Gabor - UNIV CAMBRIDGE - Reino Unido
15 Lodieu, N. Hombre Inst Astrofis Canarias - España
ULL - España
16 Marocco, F. Hombre Univ Hertfordshire - Reino Unido
17 Murray, D. N. - Univ Hertfordshire - Reino Unido
18 Sipocz, Brigitta M. Mujer Univ Hertfordshire - Reino Unido

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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: 12.0 %
Citas No-identificadas: 88.0 %

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

Citas Identificadas: 12.0 %
Citas No-identificadas: 88.0 %

Financiamiento



Fuente
FONDECYT
Spanish Ministry of Science and Innovation
CONICYT (Chile)
NSF
Science and Technology Facilities Council
Gemini Observatory
ARC
Ministerio da Ciencia e Tecnologia (Brazil)
Australian Research Council (Australia)
National Research Council (Canada)
National Science Foundation (United States)
Ministerio de Ciencia, Tecnologia e Innovacion Productiva (Argentina)
Science and Technology Facilities Council (United Kingdom)

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Agradecimientos



Agradecimiento
We thank our colleagues in the GLIMPSE360 team for providing this deep panoramic Legacy data set, which complements the UKIDSS GPS excellently. We thank Barbara Whitney, Brian Babler and Robert Benjamin for a helpful discussion of the Spitzer photometry. We thank Janet Drew for checking our candidates against the IPHAS data. This study is based on observations made under project A22TAC_96 on the Italian Telescopio Nazionale Galileo (TNG) operated on the island of La Palma by the Fundacion Galileo Galilei of the Istituto Nazionale di Astrofisica at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias and on observations obtained via program GN-2010B-Q-41 at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), Science and Technology Facilities Council (United Kingdom), National Research Council (Canada), CONICYT (Chile), Australian Research Council (Australia), Ministerio da Ciencia e Tecnologia (Brazil) and Ministerio de Ciencia, Tecnologia e Innovacion Productiva (Argentina). SKL's research is supported by the Gemini Observatory. CGT is supported by ARC grant DP0774000. ACD-J is supported by a Fondecyt postdoctorado fellowship, under project number 3100098. This research has made use of the SIMBAD data base, operated at CDS, Strasbourg, France, and has benefited from the SpeX Prism Spectral Libraries maintained by Adam Burgasser at http://www.browndwarfs.org/spexprism. JG, GK and BS are supported by RoPACS, a Marie Curie Initial Training Network funded by the European Commissions Seventh Framework Programme. NL acknowledges funding from the Spanish Ministry of Science and Innovation through the Ramon y Cajal fellowship number 08-303-01-02 and the project number AYA2010-19136. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.

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