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NPARSEC: NTT Parallaxes of Southern Extremely Cool objects. Goals, targets, procedures and first results

The discovery and subsequent detailed study of T dwarfs has provided many surprises and pushed the physics and modeling of cool atmospheres in unpredicted directions. Distance is a critical parameter for studies of these objects to determine intrinsic luminosities, test binarity and measure their motion in the Galaxy. We describe a new observational program to determine distances across the full range of T dwarf sub-types using the NTT/SOFI telescope/instrument combination. We present preliminary results for ten objects, five of which represent new distances.

preprint2013arXivOpen access
R. L. SmartC. G. TinneyB. BucciarelliF. MaroccoU. AbbasA. AndreiG. BernardiB. BurninghamC. CardosoE. CostaM. T. CrostaM. DapraA. Day-JonesB. GoldmanH. R. A. JonesM. G. LattanziS. K. LeggettP. LucasR. MendezJ. L. PennaD. PinfieldL. SmithA. SozzettiA. Vecchiato
astro-ph.IMastro-ph.SR
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Open access24 authors2 topics
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R. L. SmartC. G. TinneyB. BucciarelliF. MaroccoU. AbbasA. AndreiG. BernardiB. BurninghamC. CardosoE. CostaM. T. CrostaM. DapraA. Day-JonesB. GoldmanH. R. A. JonesM. G. LattanziS. K. LeggettP. LucasR. MendezJ. L. PennaD. PinfieldL. SmithA. SozzettiA. Vecchiato

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