A SEARCH FOR L/T TRANSITION DWARFS WITH Pan-STARRS1 AND WISE: DISCOVERY OF SEVEN NEARBY OBJECTS INCLUDING TWO CANDIDATE SPECTROSCOPIC VARIABLES

被引:31
作者
Best, William M. J. [1 ]
Liu, Michael C. [1 ]
Magnier, Eugene A. [1 ]
Aller, Kimberly M. [1 ]
Deacon, Niall R. [2 ]
Dupuy, Trent J. [3 ]
Redstone, Joshua [4 ]
Burgett, W. S. [1 ]
Chambers, K. C. [1 ]
Hodapp, K. W. [1 ]
Kaiser, N. [1 ]
Kudritzki, R-P. [1 ]
Morgan, J. S. [1 ]
Price, P. A. [5 ]
Tonry, J. L. [1 ]
Wainscoat, R. J. [1 ]
机构
[1] Univ Hawaii Manoa, Inst Astron, Honolulu, HI 96822 USA
[2] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[4] Facebook, New York, NY 10017 USA
[5] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
binaries: general; brown dwarfs; stars: atmospheres; stars: individual (PSO J140.2308+45.6487; PSO J307.6784+07.8236); stars: variables: general; STAR ADAPTIVE OPTICS; DIGITAL SKY SURVEY; SPECTRAL TYPE-L; T-DWARF; BROWN DWARF; PHOTOMETRIC VARIABILITY; COOL NEIGHBORS; DYNAMICAL MASS; LUMINOSITY FUNCTION; ULTRACOOL DWARFS;
D O I
10.1088/0004-637X/777/2/84
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present initial results from a wide-field (30,000 deg(2)) search for L/T transition brown dwarfs within 25 pc using the Pan-STARRS1 and Wide-field Infrared Survey Explorer (WISE) surveys. Previous large-area searches have been incomplete for L/T transition dwarfs, because these objects are faint in optical bands and have near-infrared (near-IR) colors that are difficult to distinguish from background stars. To overcome these obstacles, we have cross-matched the Pan-STARRS1 (optical) and WISE (mid-IR) catalogs to produce a unique multi-wavelength database for finding ultracool dwarfs. As part of our initial discoveries, we have identified seven brown dwarfs in the L/T transition within 9-15 pc of the Sun. The L9.5 dwarf PSO J140.2308+45.6487 and the T1.5 dwarf PSO J307.6784+07.8263 (both independently discovered by Mace et al.) show possible spectroscopic variability at the Y and J bands. Two more objects in our sample show evidence of photometric J-band variability, and two others are candidate unresolved binaries based on their spectra. We expect our full search to yield a well-defined, volume-limited sample of L/T transition dwarfs that will include many new targets for study of this complex regime. PSO J307.6784+07.8263 in particular may be an excellent candidate for in-depth study of variability, given its brightness (J = 14.2 mag) and proximity (11 pc).
引用
收藏
页数:13
相关论文
共 97 条
[1]   The first data release of the Sloan Digital Sky Survey [J].
Abazajian, K ;
Adelman-McCarthy, JK ;
Agüeros, MA ;
Allam, SS ;
Anderson, SF ;
Annis, J ;
Bahcall, NA ;
Baldry, IK ;
Bastian, S ;
Berlind, A ;
Bernardi, M ;
Blanton, MR ;
Blythe, N ;
Bochanski, JJ ;
Boroski, WN ;
Brewington, H ;
Briggs, JW ;
Brinkmann, J ;
Brunner, RJ ;
Budavári, T ;
Carey, LN ;
Carr, MA ;
Castander, FJ ;
Chiu, K ;
Collinge, MJ ;
Connolly, AJ ;
Covey, KR ;
Csabai, I ;
Dalcanton, JJ ;
Dodelson, S ;
Doi, M ;
Dong, F ;
Eisenstein, DJ ;
Evans, ML ;
Fan, XH ;
Feldman, PD ;
Finkbeiner, DP ;
Friedman, SD ;
Frieman, JA ;
Fukugita, M ;
Gal, RR ;
Gillespie, B ;
Glazebrook, K ;
Gonzalez, CF ;
Gray, J ;
Grebel, EK ;
Grodnicki, L ;
Gunn, JE ;
Gurbani, VK ;
Hall, PB .
ASTRONOMICAL JOURNAL, 2003, 126 (04) :2081-2086
[2]   WISE/2MASS-SDSS brown dwarfs candidates using Virtual Observatory tools [J].
Aberasturi, M. ;
Solano, E. ;
Martin, E. L. .
ASTRONOMY & ASTROPHYSICS, 2011, 534
[3]   Precipitating condensation clouds in substellar atmospheres [J].
Ackerman, AS ;
Marley, MS .
ASTROPHYSICAL JOURNAL, 2001, 556 (02) :872-884
[4]   The limiting effects of dust in brown dwarf model atmospheres [J].
Allard, F ;
Hauschildt, PH ;
Alexander, DR ;
Tamanai, A ;
Schweitzer, A .
ASTROPHYSICAL JOURNAL, 2001, 556 (01) :357-372
[5]   Star formation via the little guy: A Bayesian study of ultracool dwarf imaging surveys for companions [J].
Allen, Peter R. .
ASTROPHYSICAL JOURNAL, 2007, 668 (01) :492-506
[6]   A new brown dwarf desert? A scarcity of wide ultracool binaries [J].
Allen, Peter R. ;
Koerner, David W. ;
McElwain, Michael W. ;
Cruz, Kelle L. ;
Reid, I. Neill .
ASTRONOMICAL JOURNAL, 2007, 133 (03) :971-978
[7]  
[Anonymous], YCAT
[8]   HST SPECTRAL MAPPING OF L/T TRANSITION BROWN DWARFS REVEALS CLOUD THICKNESS VARIATIONS [J].
Apai, Daniel ;
Radigan, Jacqueline ;
Buenzli, Esther ;
Burrows, Adam ;
Reid, Iain Neill ;
Jayawardhana, Ray .
ASTROPHYSICAL JOURNAL, 2013, 768 (02)
[9]   PHOTOMETRIC VARIABILITY OF THE T2.5 BROWN DWARF SIMP J013656.5+093347: EVIDENCE FOR EVOLVING WEATHER PATTERNS [J].
Artigau, Etienne ;
Bouchard, Sandie ;
Doyon, Rene ;
Lafreniere, David .
ASTROPHYSICAL JOURNAL, 2009, 701 (02) :1534-1539
[10]   Spectroscopic rotation velocities of L dwarfs from VLT/UVES and their comparison with periods from photometric monitoring [J].
Bailer-Jones, CAL .
ASTRONOMY & ASTROPHYSICS, 2004, 419 (02) :703-712