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20002024
most citedThe UKIRT Infrared Deep Sky Survey (UKIDSS)

2.5k citations · 12.7k across the 122 of their papers we have counts for

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Showing 2013Show all

10 papers · 1 filter

astro-ph.EP2013★ 175 cited

A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic Bulge

D. P. Bennett, V. Batista, I. A. Bond +90

We present the first microlensing candidate for a free-floating exoplanet-exomoon system, MOA-2011-BLG-262, with a primary lens mass of M_host ~ 4 Jupiter masses hosting a sub-Eart…

astro-ph.SR2013★ 12 cited

Stellar Variability in the VVV survey

M. Catelan, D. Minniti, P. W. Lucas +34

The Vista Variables in the Vía Láctea (VVV) ESO Public Survey is an ongoing time-series, near-infrared (IR) survey of the Galactic bulge and an adjacent portion of the inner disk,…

astro-ph.SR2013★ 3 cited

Multi-Object and Long-Slit Spectroscopy of Very Low Mass Brown Dwarfs in Orion Nebular Cluster

Takuya Suenaga, Motohide Tamura, Masayuki Kuzuhara +3

We present the results of a H- and K-band multi-object and long-slit spectroscopic survey of substellar mass candidates in the outer regions of the Orion Nebula Cluster. The spectr…

astro-ph.SR2013★ 68 cited

Parallaxes of Southern Extremely Cool objects (PARSEC) II: Spectroscopic Follow-up and Parallaxes of 52 Targets

F. Marocco, A. H. Andrei, R. L. Smart +8

We present near-infrared spectroscopy for 52 ultracool dwarfs, including two newly discovered late-M dwarfs, one new late-M subdwarf candidate, three new L and four new T dwarfs. W…

astro-ph.SR2013★ 35 cited

One more neighbor: The first brown dwarf in the VVV survey

J. C. Beamín, D. Minniti, M. Gromadzki +6

Context. The discovery of brown dwarfs (BDs) in the solar neighborhood and young star clusters has helped to constraint the low-mass end of the stellar mass function and the initia…

astro-ph.GA2013★ 38 cited

A deep WISE search for very late type objects and the discovery of two halo/thick-disk T dwarfs: WISE 0013+0634 and WISE 0833+0052

D. J. Pinfield, J. Gomes, A. C. Day-Jones +21

A method is defined for identifying late T and Y dwarfs in WISE down to low values of signal-to-noise. This requires a WISE detection only in the W2-band and uses the statistical p…