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| 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
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.
| 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 |
| 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 |
| 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. |