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High proper motion objects from the UKIDSS Galactic plane survey
Indexado
WoS WOS:000342920400031
Scopus SCOPUS_ID:84906070113
DOI 10.1093/MNRAS/STU1295
Año 2014
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



The UKIDSS Galactic Plane Survey (GPS) began in 2005 as a seven year effort to survey similar to 1800 deg(2) of the northern Galactic plane in the J, H, and K passbands. The survey included a second epoch of K-band data, with a baseline of two to eight years, for the purpose of investigating variability and measuring proper motions. We have calculated proper motions for 167 million sources in a 900 deg(2) area located at l > 60 degrees. in order to search for new high proper motion objects. Visual inspection has verified 617 high proper motion sources (>200 mas yr(-1)) down to K = 17, of which 153 are new discoveries. Among these, we have a new spectroscopically confirmed T5 dwarf, an additional T dwarf with estimated type T6, 13 new L dwarf candidates, and two new common proper motion systems containing ultracool dwarf candidates. We provide improved proper motions for an additional 12 high proper motion stars that were independently discovered in the WISE data set during the course of this investigation.

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
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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 Smith, L. C. Mujer Univ Hertfordshire - Reino Unido
University of Hertfordshire - Reino Unido
2 Lucas, Philip Hombre Univ Hertfordshire - Reino Unido
University of Hertfordshire - Reino Unido
3 Bunce, R. - Univ Hertfordshire - Reino Unido
University of Hertfordshire - Reino Unido
4 Burningham, B. Hombre Univ Hertfordshire - Reino Unido
University of Hertfordshire - Reino Unido
5 Jones, Hugh R. A. Hombre Univ Hertfordshire - Reino Unido
University of Hertfordshire - Reino Unido
6 Smart, R. L. Hombre Osservatorio Astrofis Torino - Italia
Istituto Nazionale Di Astrofisica, Rome - Italia
7 Skrzypek, N. - Univ London Imperial Coll Sci Technol & Med - Reino Unido
Imperial College London - Reino Unido
8 Rodriguez, David Hombre Universidad de Chile - Chile
9 Faherty, Jacqueline Mujer Carnegie Inst Sci - Estados Unidos
Carnegie Institution of Washington - Estados Unidos
10 Luciano, Juan Francisco Lagos Hombre Univ Hertfordshire - Reino Unido
11 Drew, J. Mujer Univ Hertfordshire - Reino Unido
University of Hertfordshire - Reino Unido
12 Andrei, A. - Univ Hertfordshire - Reino Unido
MCTI - Brasil
UNIV FED RIO DE JANEIRO - Brasil
University of Hertfordshire - Reino Unido
Observatório Nacional - Brasil
Universidade Federal do Rio de Janeiro - Brasil
13 CATALAN-HOTT, SUSAN ROSSEMARIE Mujer Univ Warwick - Reino Unido
The University of Warwick - Reino Unido
Faculty of Science, Engineering and Medicine - Reino Unido
14 Pinfield, David J. Hombre Univ Hertfordshire - Reino Unido
University of Hertfordshire - Reino Unido
15 Redburn, D. - Univ Hertfordshire - Reino Unido
University of 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: 29.41 %
Citas No-identificadas: 70.59 %

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

Citas Identificadas: 29.41 %
Citas No-identificadas: 70.59 %

Financiamiento



Fuente
FONDECYT
CNPq
STFC
Science and Technology Facilities Council
Seventh Framework Programme
Marie Curie 7th European Community Framework Programme
Science & Technology Facilities Research Council (STFC) of the UK
Nuffield Foundation

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Agradecimientos



Agradecimiento
We would like to thank the referee, John Gizis, for a very positive review. LS acknowledges a studentship funded by the Science & Technology Facilities Research Council (STFC) of the UK; PWL, PP, DJP, GB, JED acknowledge the support of a consolidated grant (ST/J001333/1) also funded by STFC. This work is based in part on data obtained as part of the UKIRT Infrared Deep Sky Survey. The authors would like to acknowledge the Marie Curie 7th European Community Framework Programme grant no. 247593 Interpretation and Parametrization of Extremely Red COOL dwarfs (IPERCOOL) International Research Staff Exchange Scheme. AHA acknowledges CNPq grant PQ306775/2009-3. DRR acknowledges support from FONDECYT grant 3130520. This research has made use of the SIMBAD data base and VizieR catalogue access tool, operated at CDS, Strasbourg, France. This research has made use of NASA's Astrophysics Data System Bibliographic Services. This research has made use of SAOImage DS9, developed by Smithsonian Astrophysical Observatory. This research has made use of the SpeX Spectrograph and Imager on the NASA Infrared Telescope Facility, see Rayner et al. (2003). The authors would like to acknowledge Setpoint Hertfordshire and the Nuffield Foundation for organizing and funding the research placement of R. Bunce.

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