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Fifteen new T dwarfs discovered in the UKIDSS Large Area Survey

Identifieur interne : 000D58 ( Istex/Curation ); précédent : 000D57; suivant : 000D59

Fifteen new T dwarfs discovered in the UKIDSS Large Area Survey

Auteurs : D. J. Pinfield [Royaume-Uni] ; B. Burningham ; M. Tamura [Japon] ; S. K. Leggett [États-Unis] ; N. Lodieu [Espagne] ; P. W. Lucas ; D. J. Mortlock ; S. J. Warren ; D. Homeier [Allemagne] ; M. Ishii [États-Unis] ; N. R. Deacon [Pays-Bas] ; R. G. Mcmahon ; P. C. Hewett ; M. R. Zapatero Osori [Espagne] ; E. L. Martin [Espagne] ; H. R. A. Jones ; B. P. Venemans ; A. C. Day-Jones ; P. D. Dobbie [Australie] ; S. L. Folkes ; S. Dye ; F. Allard [France] ; I. Baraffe [France] ; D. Barrado Y Navascués [Espagne] ; S. L. Casewell ; K. Chiu ; G. Chabrier [France] ; F. Clarke [Chili] ; S. T. Hodgkin ; A. Magazzù [Espagne] ; M. J. Mccaughrean ; T. Nakajima [Japon] ; Y. Pavlenko [Ukraine] ; C. G. Tinney [Australie]

Source :

RBID : ISTEX:486B8773293118A6D1EC9DCCE7E16884CAAF569C

Abstract

We present the discovery of 15 new T2.5–T7.5 dwarfs (with estimated distances ∼24–93 pc), identified in the first three main data releases of the United Kingdom Infrared Telescope (UKIRT) Infrared Deep Sky Survey. This brings the total number of T dwarfs discovered in the Large Area Survey (LAS) (to date) to 28. These discoveries are confirmed by near-infrared spectroscopy, from which we derive spectral types on the unified scheme of Burgasser et al. Seven of the new T dwarfs have spectral types of T2.5–T4.5, five have spectral types of T5–T5.5, one is a T6.5p and two are T7–7.5. We assess spectral morphology and colours to identify T dwarfs in our sample that may have non-typical physical properties (by comparison to solar neighbourhood populations), and find that three of these new T dwarfs may have unusual metallicity, two may have low surface gravity, and one may have high surface gravity. The colours of the full sample of LAS T dwarfs show a possible trend to bluer Y−J with decreasing effective temperature, and some interesting colour changes in J−H and z−J (deserving further investigation) beyond T8. The LAS T dwarf sample from the first and second main data releases show good evidence for a good level of completion to J= 19. By accounting for the main sources of incompleteness (selection, follow-up and spatial) as well as the effects of unresolved binarity, Malmquist and Eddington bias, we estimate that there are 17 ± 4 ≥ T 4 dwarfs in the J≤ 19 volume of the LAS second data release. This value is most consistent with theoretical predictions if the substellar mass function exponent α (dN/dm∝m−α) lies between −1.0 and 0. This is consistent with the latest 2-Micron All Sky Survey (2MASS)/Sloan Digital Sky Survey (SDSS) constraint (which is based on lower number statistics) and is significantly lower than the α∼ 1.0 suggested by L dwarf field populations, which is possibly a result of the lower mass range probed by the T dwarf class.

Url:
DOI: 10.1111/j.1365-2966.2008.13729.x

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D. J. Pinfield
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B. Burningham
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P. W. Lucas
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D. J. Mortlock
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S. J. Warren
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R. G. Mcmahon
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P. C. Hewett
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H. R. A. Jones
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B. P. Venemans
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A. C. Day-Jones
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S. L. Folkes
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S. Dye
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S. L. Casewell
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K. Chiu
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<name sortKey="Nakajima, T" sort="Nakajima, T" uniqKey="Nakajima T" first="T." last="Nakajima">T. Nakajima</name>
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<name sortKey="Tinney, C G" sort="Tinney, C G" uniqKey="Tinney C" first="C. G." last="Tinney">C. G. Tinney</name>
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<mods:affiliation>Department of Astrophysics, University of New South Wales, Sydney, NSW 2052, Australia</mods:affiliation>
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<title level="j">Monthly Notices of the Royal Astronomical Society</title>
<title level="j" type="abbrev">Monthly Notices of the Royal Astronomical Society</title>
<idno type="ISSN">0035-8711</idno>
<idno type="eISSN">1365-2966</idno>
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<publisher>Blackwell Publishing Ltd</publisher>
<pubPlace>Oxford, UK</pubPlace>
<date type="published" when="2008-10-11">2008-10-11</date>
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<div type="abstract">We present the discovery of 15 new T2.5–T7.5 dwarfs (with estimated distances ∼24–93 pc), identified in the first three main data releases of the United Kingdom Infrared Telescope (UKIRT) Infrared Deep Sky Survey. This brings the total number of T dwarfs discovered in the Large Area Survey (LAS) (to date) to 28. These discoveries are confirmed by near-infrared spectroscopy, from which we derive spectral types on the unified scheme of Burgasser et al. Seven of the new T dwarfs have spectral types of T2.5–T4.5, five have spectral types of T5–T5.5, one is a T6.5p and two are T7–7.5. We assess spectral morphology and colours to identify T dwarfs in our sample that may have non-typical physical properties (by comparison to solar neighbourhood populations), and find that three of these new T dwarfs may have unusual metallicity, two may have low surface gravity, and one may have high surface gravity. The colours of the full sample of LAS T dwarfs show a possible trend to bluer Y−J with decreasing effective temperature, and some interesting colour changes in J−H and z−J (deserving further investigation) beyond T8. The LAS T dwarf sample from the first and second main data releases show good evidence for a good level of completion to J= 19. By accounting for the main sources of incompleteness (selection, follow-up and spatial) as well as the effects of unresolved binarity, Malmquist and Eddington bias, we estimate that there are 17 ± 4 ≥ T 4 dwarfs in the J≤ 19 volume of the LAS second data release. This value is most consistent with theoretical predictions if the substellar mass function exponent α (dN/dm∝m−α) lies between −1.0 and 0. This is consistent with the latest 2-Micron All Sky Survey (2MASS)/Sloan Digital Sky Survey (SDSS) constraint (which is based on lower number statistics) and is significantly lower than the α∼ 1.0 suggested by L dwarf field populations, which is possibly a result of the lower mass range probed by the T dwarf class.</div>
</front>
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