Paul Roche

TL;DR: The paper as discussed by the authors was published in the Monthly Notices of the Royal Astronomical Society (MNO) by the British Astronomical Association (BAA) and Blackwell Publishing, London, UK.

TL;DR: In this article, the authors were partially supported by grantsAYA2008-06166-C03-03 and Consolider-GTCCSD-2006-00070 from the Spanish Ministerio de Ciencia e Innovacion (MICINN).

TL;DR: In this paper, a double-peaked outburst of an accreting milli-second X-ray pulsar (AMXP), IGR J00291+5934, underwent an outburst lasting ∼100 days, the first since its discovery in 2004.

TL;DR: In this article, a detailed morphological and photometric characterisation of Comet 29P in the optical region is presented comprising: (a) multi-filter observations of the outburst coma in 2010-2012 with the 2.0m Faulkes Telescopes (FT); (b) high-cadence, high-precision photometry in May-September 2014; and (c) HST observations in March 1996 (WFPC2/F702W filter).

TL;DR: In this article, three years of optical monitoring of the low-mass X-ray binary (LMXB) 4U 1957+11 is presented, where the light curve is dominated by long-term variations which are correlated (at the >3σ level) with the soft Xray flux from the All Sky Monitor on board the Rossi X-Ray Timing Explorer, and the authors find no evidence for periodicities in their light curves, contrary to a previous short-time-scale optical study in which the flux varied on a 9.3-h sinusoidal