Two T dwarfs from the UKIDSS early data release

被引:33
作者
Kendall, T. R.
Tamura, M.
Tinney, C. G.
Martin, E. L.
Ishii, M.
Pinfield, D. J.
Lucas, P. W.
Jones, H. R. A.
Leggett, S. K.
Dye, S.
Hewett, P. C.
Allard, F.
Baraffe, I.
Navascues, D. Barrado Y.
Carraro, G.
Casewell, S. L.
Chabrier, G.
Chappelle, R. J.
Clarke, F.
Day-Jones, A.
Deacon, N.
Dobbie, P. D.
Folkes, S.
Hambly, N. C.
Hodgkin, S. T.
Nakajima, T.
Jameson, R. F.
Lodieu, N.
Magazzu, A.
McCaughrean, M. J.
Pavlenko, Y. V.
Tadashi, N.
Osorio, M. R. Zapatero
机构
[1] Univ Hertfordshire, Ctr Astrophys Res, Sci & Technol Res Inst, Hatfield AL10 9AB, Herts, England
[2] Natl Astron Observ, Mitaka, Tokyo 1818588, Japan
[3] Anglo Australian Observ, Epping, NSW 1710, Australia
[4] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Spain
[5] Univ Cent Florida, Dept Phys, Orlando, FL 32816 USA
[6] Subaru Telescope, Hilo, HI 96720 USA
[7] Gemini Observ, Hilo, HI 96720 USA
[8] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales
[9] Inst Astron, Cambridge CB3 0HA, England
[10] Ecole Normale Super Lyon, CRAL, UMR 5574, CNRS, F-69364 Lyon, France
[11] INTA, Lab Astrofis Espacial & Fis Fundamental, Madrid 28080, Spain
[12] Univ Padua, Dipartimento Astron, I-35122 Padua, Italy
[13] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[14] Acad Sci Czech Republic, Inst Astron, Prague 14131, Czech Republic
[15] European So Observ, Santiago 19, Chile
[16] Univ Edinburgh, Royal Observ, Scottish Univ Phys Alliance, Inst Astron,Sch Phys, Edinburgh EH9 3HJ, Midlothian, Scotland
[17] Fdn Galileo Galilei INAF, Santa Cruz de la Palma 38700, Spain
[18] Univ Exeter, Sch Phys, Exeter EX4 4QL, Devon, England
[19] Natl Acad Sci Ukraine, Main Astron Observ, UA-03680 Kiev, Ukraine
[20] Radboud Univ Nijmegen, Dept Astrophys, Fac Sci, NL-6500 GL Nijmegen, Netherlands
基金
英国科学技术设施理事会;
关键词
infrared : stars; stars; low-mass; brown dwarfs; stars : fundamental parameters;
D O I
10.1051/0004-6361:20066403
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Context. We report on the first ultracool dwarf discoveries from the UKIRT Infrared Deep Sky Survey ( UKIDSS) Large Area Survey Early Data Release ( LAS EDR), in particular the discovery of T dwarfs which are fainter and more distant than those found using the 2MASS and SDSS surveys. Aims. We aim to show that our methodologies for searching the similar to 27 deg(2) of the LAS EDR are successful for finding both L and T dwarfs via cross-correlation with the Sloan Digital Sky Survey ( SDSS) DR4 release. While the area searched so far is small, the numbers of objects found shows great promise for near-future releases of the LAS and great potential for finding large numbers of such dwarfs. Methods. Ultracool dwarfs are selected by combinations of their YJH(K) UKIDSS colours and SDSS DR4 z - J and i - z colours, or, lower limits on these red optical/infrared colours in the case of DR4 dropouts. After passing visual inspection tests, candidates have been followed up by methane imaging and spectroscopy at 4 m and 8m-class facilities. Results. Our main result is the discovery following CH4 imaging and spectroscopy of a T4.5 dwarf, ULAS J 1452+0655, lying similar to 80 pc distant. A further T dwarf candidate, ULAS J 1301+0023, has very similar CH4 colours but has not yet been confirmed spectroscopically. We also report on the identification of a brighter L0 dwarf, and on the selection of a list of LAS objects designed to probe for T-like dwarfs to the survey J-band limit. Conclusions. Our findings indicate that the combination of the UKIDSS LAS and SDSS surveys provide an excellent tool for identifying L and T dwarfs down to much fainter limits than previously possible. Our discovery of one confirmed and one probable T dwarf in the EDR is consistent with expectations from the previously measured T dwarf density on the sky.
引用
收藏
页码:1059 / 1064
页数:6
相关论文
共 18 条
[1]   A unified near-infrared spectral classification scheme for T dwarfs [J].
Burgasser, AJ ;
Geballe, TR ;
Leggett, SK ;
Kirkpatrick, JD ;
Golimowski, DA .
ASTROPHYSICAL JOURNAL, 2006, 637 (02) :1067-1093
[2]   Galactic stellar and substellar initial mass function [J].
Chabrier, G .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2003, 115 (809) :763-795
[3]  
Chabrier G, 2005, ASTROPHYS SPACE SC L, V327, P41
[4]   The Galactic disk mass budget. II. Brown dwarf mass function and density [J].
Chabrier, G .
ASTROPHYSICAL JOURNAL, 2002, 567 (01) :304-313
[5]   Seventy-one new L and T dwarfs from the Sloan Digital Sky Survey [J].
Chiu, K ;
Fan, X ;
Leggett, SK ;
Golimowski, DA ;
Zheng, W ;
Geballe, TR ;
Schneider, DP ;
Brinkmann, J .
ASTRONOMICAL JOURNAL, 2006, 131 (05) :2722-2736
[6]   Meeting the cool neighbors. V. A 2MASS-selected sample of ultracool dwarfs [J].
Cruz, KL ;
Reid, IN ;
Liebert, J ;
Kirkpatrick, JD ;
Lowrance, PJ .
ASTRONOMICAL JOURNAL, 2003, 126 (05) :2421-2448
[7]  
Cuby JG, 1999, ASTRON ASTROPHYS, V349, pL41
[8]   An infrared spectroscopic sequence of M, L, and T dwarfs [J].
Cushing, MC ;
Rayner, JT ;
Vacca, WD .
ASTROPHYSICAL JOURNAL, 2005, 623 (02) :1115-1140
[9]   The possiblity of detection of ultracool dwarfs with the UKIRT Infrared Deep Sky Survey [J].
Deacon, N. R. ;
Hambly, N. C. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 371 (04) :1722-1730
[10]   The UKIRT Infrared Deep Sky Survey Early Data Release [J].
Dye, S. ;
Warren, S. J. ;
Hambly, N. C. ;
Cross, N. J. G. ;
Hodgkin, S. T. ;
Irwin, M. J. ;
Lawrence, A. ;
Adamson, A. J. ;
Almaini, O. ;
Edge, A. C. ;
Hirst, P. ;
Jameson, R. F. ;
Lucas, P. W. ;
van Breukelen, C. ;
Bryant, J. ;
Casali, M. ;
Collins, R. S. ;
Dalton, G. B. ;
Davies, J. I. ;
Davis, C. J. ;
Emerson, J. P. ;
Evans, D. W. ;
Foucaud, S. ;
Gonzales-Solares, E. A. ;
Hewett, P. C. ;
Kendall, T. R. ;
Kerr, T. H. ;
Leggett, S. K. ;
Lodieu, N. ;
Loveday, J. ;
Lewis, J. R. ;
Mann, R. G. ;
McMahon, R. G. ;
Mortlock, D. J. ;
Nakajima, Y. ;
Pinfield, D. J. ;
Rawlings, M. G. ;
Read, M. A. ;
Riello, M. ;
Sekiguchi, K. ;
Smith, A. J. ;
Sutorius, E. T. W. ;
Varricatt, W. ;
Walton, N. A. ;
Weatherley, S. J. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 372 (03) :1227-1252