activity
20052009
most citedThe discovery of an M4+T8.5 binary system

125 citations · 391 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA200953 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.SR2009125 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-ph200889 cited

Fifteen new T dwarfs discovered in the UKIDSS Large Area Survey

D. J. Pinfield, B. Burningham, M. Tamura +32

We present the discovery of fifteen new T2.5-T7.5 dwarfs (with estimated distances between ~24-93pc, identified in the first three main data releases of the UKIRT Infrared Deep Sky…

astro-ph2008124 cited

Exploring the substellar temperature regime down to ~550K

Ben Burningham, D. J. Pinfield, S. K. Leggett +15

We report the discovery of three very late T dwarfs in the UKIRT Infrared Deep Sky Survey (UKIDSS) Third Data Release: ULAS J101721.40+011817.9 (ULAS1017), ULAS J123828.51+095351.3…

astro-ph2005

Can variability account for apparent age spreads in OB association colour-magnitude diagrams?

Ben Burningham, Tim Naylor, S. P. Littlefair +1

We have investigated the role of photometric variability in causing the apparent age spreads observed in the colour-magnitude diagrams of OB associations. We have found that the co…

astro-ph2005

Do accretion discs regulate the rotation of young stars?

S. P. Littlefair, Tim Naylor, Ben Burningham +1

We present a photometric study of I-band variability in the young cluster IC 348. The main purpose of the study was to identify periodic stars. In all we find 50 periodic stars, of…