activity
20062016
most citedRapid formation of large dust grains in the luminous supernova SN 2010jl

219 citations · 2.8k across the 50 of their papers we have counts for

collaborators

50 papers

astro-ph.SR2016★ 78 cited

Primeval very low-mass stars and brown dwarfs. I. Six new L subdwarfs, classification and atmospheric properties

Z. H. Zhang, D. J. Pinfield, M. C. Galvez-Ortiz +10

We have conducted a search for L subdwarf candidates within the photometric catalogues of the UKIRT Infrared Deep Sky Survey and Sloan Digital Sky Survey. Six of our candidates are…

astro-ph.EP2016★ 65 cited

New Planetary Systems from the Calan-Hertfordshire Extrasolar Planet Search

J. S. Jenkins, H. R. A. Jones, M. Tuomi +22

We report the discovery of eight new giant planets, and updated orbits for four known planets, orbiting dwarf and subgiant stars using the CORALIE, HARPS, and MIKE instruments as p…

astro-ph.SR2016★ 15 cited

A Method for Selecting M dwarfs with an Increased Likelihood of Unresolved Ultra-cool Companionship

N. J. Cook, D. J. Pinfield, F. Marocco +15

Locating ultra-cool companions to M dwarfs is important for constraining low-mass formation models, the measurement of sub-stellar dynamical masses and radii, and for testing ultra…

astro-ph.SR2015★ 89 cited

A large spectroscopic sample of L and T dwarfs from UKIDSS LAS: peculiar objects, binaries, and space density

F. Marocco, H. R. A. Jones, A. C. Day-Jones +7

We present the spectroscopic analysis of a large sample of late-M, L, and T dwarfs from UKIDSS. Using the YJHK photometry from ULAS and the red-optical photometry from SDSS we sele…

astro-ph.SR2014★ 36 cited

Discovery of a new Y dwarf: WISE J030449.03-270508.3

D. J. Pinfield, M. Gromadzki, S. K. Leggett +21

We present a new Y dwarf, WISE J030449.03-270508.3, confirmed from a candidate sample designed to pick out low temperature objects from the WISE database. The new object is typed Y…

astro-ph.SR2014★ 219 cited

Rapid formation of large dust grains in the luminous supernova SN 2010jl

Christa Gall, Jens Hjorth, Darach Watson +6

The origin of dust in galaxies is still a mystery. The majority of the refractory elements are produced in supernova explosions but it is unclear how and where dust grains condense…