activity
20042026
most citedDiscovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager

559 citations · 4.5k across the 92 of their papers we have counts for

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Showing 2009Show all

6 papers · 1 filter

astro-ph.SR2009★ 2 cited

The current population of benchmark brown dwarfs

A. C. Day-Jones, D. J. Pinfield, M. T. Ruiz +7

The number of brown dwarfs (BDs) now identified tops 700. Yet our understanding of these cool objects is still lacking, and models are struggling to accurately reproduce observatio…

astro-ph.SR2009★ 32 cited

The distance to the cool T9 brown dwarf ULAS J003402.77-005206.7

R. L. Smart, H. R. A. Jones, M. G. Lattanzi +8

Aims. We demonstrate the feasibility of determining parallaxes for nearby objects with theWide Field Camera on the United Kingdom Infrared Telescope (UKIRT) using the UKIRT Infrare…

astro-ph.SR2009

Benchmark ultra-cool dwarfs in widely separated binary systems

Z. H. Zhang, D. J. Pinfield, A. C. Day-Jones +2

Ultra-cool dwarfs as wide companions to subgiants, giants, white dwarfs and main sequence stars can be very good benchmark objects, for which we can infer physical properties with…

astro-ph.GA2009★ 53 cited

Ultra-cool dwarfs: new discoveries, proper motions, and improved spectral typing from SDSS and 2MASS photometric colors

Z. H. Zhang, R. S. Pokorny, H. R. A. Jones +6

Aims. We try to identify ultra-cool dwarfs from the seventh Data Release of the Sloan Digital Sky Survey (SDSS DR7) with SDSS i-z and r-z colors. We also obtain proper motion data…

astro-ph.SR2009★ 125 cited

The discovery of an M4+T8.5 binary system

Ben Burningham, D. J. Pinfield, S. K. Leggett +17

We report the discovery of a T8.5 dwarf, which is a companion to the M4 dwarf Wolf 940. At a distance of 12.50 (+0.75,-0.67) pc, the angular separation of 32arcsec corresponds to a…

astro-ph.SR2009★ 88 cited

The Physical Properties of Four ~600K T Dwarfs

S. K. Leggett, M. C. Cushing, D. Saumon +16

We present Spitzer 7.6-14.5um spectra of ULAS J003402.77-005206.7 and ULAS J133553.45+113005.2, two T9 dwarfs with the latest spectral types currently known. We fit synthetic spect…