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20032008
most citedRapid optical and X-ray timing observations of GX 339-4: flux correlations at the onset of a low/hard state

97 citations · 198 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph200897 cited

Rapid optical and X-ray timing observations of GX 339-4: flux correlations at the onset of a low/hard state

P. Gandhi, K. Makishima, M. Durant +6

We present the discovery of optical/X-ray flux correlations on rapid timescales in the low/hard state of the Galactic black hole GX 339-4. The source had recently emerged from outb…

astro-ph200740 cited

Observations of the 599 Hz Accreting X-ray Pulsar IGR J00291+5934 during the 2004 Outburst and in Quiescence

M. A. P. Torres, P. G. Jonker, D. Steeghs +10

We report on optical and NIR observations obtained during and after the 2004 December discovery outburst of the X-ray transient and accretion-powered millisecond pulsar IGR J00291+…

astro-ph200661 cited

The periodic variations of a white-light flare observed with ULTRACAM

M. Mathioudakis, D. S. Bloomfield, D. B. Jess +2

High time resolution observations of a white--light flare on the active star EQ PegB show evidence of intensity variations with a period of approximately 10 s. The period drifts to…

astro-ph2003

Mass Transfer between Double White Dwarfs

T. R. Marsh, G. Nelemans, D. Steeghs

Three periodically variable stars have recently been discovered (V407 Vul, P=9.5 min; ES Cet, P=10.3 min; RX J0806.3+1527, P=5.3 min) with properties that suggest that their photom…

astro-ph2003

Photometric variability of the unique magnetic white dwarf GD356

C. S. Brinkworth, M. R. Burleigh, G. A. Wynn +1

GD356 is a magnetic white dwarf (B = 13MG) that uniquely displays weak resolved Zeeman triplets of Halpha and Hbeta in emission. As such, GD356 may be the only known white dwarf wi…

astro-ph2003

The orbital period distribution of subdwarf B binaries

L. Morales-Rueda, P. F. L. Maxted, T. R. Marsh

We present the results of a 3.5 year long campaign to measure orbital periods of subdwarf B (sdB) star binaries. We directly compare our observed orbital period distribution with t…