activity
20012009
most citedULTRACAM: an ultra-fast, triple-beam CCD camera for high-speed astrophysics

343 citations · 963 across the 14 of their papers we have counts for

collaborators
Showing astro-phShow all

22 papers · 1 filter

astro-ph200827 cited

ULTRACAM observations of two accreting white dwarf pulsators

C. M. Copperwheat, T. R. Marsh, V. S. Dhillon +6

In this paper we present high time-resolution observations of GW Librae and SDSS J161033.64-010223.3 -- two cataclysmic variables which have shown periodic variations attributed to…

astro-ph200832 cited

Optical variability of the ultracool dwarf TVLM 513-46546: evidence for inhomogeneous dust clouds

S. P. Littlefair, V. S. Dhillon, T. R. Marsh +3

We present multi-colour photometry of the M8.5V ultracool dwarf "pulsar" TVLM 513-46546 (hereafter TVLM 513) obtained with the triple-beam photometer ULTRACAM. Data were obtained s…

astro-ph2008144 cited

On the evolutionary status of short period cataclysmic variables

S. P. Littlefair, V. S. Dhillon, T. R. Marsh +5

(Abridged) We present high-speed, three-colour photometry of seven short period (Porb <= 95 mins) eclipsing CVs from the Sloan Digital Sky Survey. We determine the system parameter…

astro-ph2007343 cited

ULTRACAM: an ultra-fast, triple-beam CCD camera for high-speed astrophysics

V. S. Dhillon, T. R. Marsh, M. J. Stevenson +15

ULTRACAM is a portable, high-speed imaging photometer designed to study faint astronomical objects at high temporal resolutions. ULTRACAM employs two dichroic beamsplitters and thr…

astro-ph200690 cited

A brown dwarf mass donor in an accreting binary

S. P. Littlefair, V. S. Dhillon, T. R. Marsh +3

A long standing and unverified prediction of binary star evolution theory is the existence of a population of white dwarfs accreting from sub-stellar donor stars. Such systems ough…

astro-ph200689 cited

Empirical isochrones and relative ages for young stars, and the radiative-convective gap

N. J. Mayne, Tim Naylor, S. P. Littlefair +2

We have selected pre-main-sequence stars in 12 groups of notional ages ranging from 1 Myr to 35 Myrs, using heterogeneous membership criteria. Using these members we have construct…