activity
19992018
most citedInvestigating the Rotational Phase of Stellar Flares on M dwarfs Using K2 Short Cadence Data

67 citations · 94 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2018★ 67 cited

Investigating the Rotational Phase of Stellar Flares on M dwarfs Using K2 Short Cadence Data

L. Doyle, G. Ramsay, J. G. Doyle +2

We present an analysis of K2 short cadence data of 34 M dwarfs which have spectral types in the range M0 - L1. Of these stars, 31 showed flares with a duration between 10-90…

astro-ph.HE2017★ 7 cited

A Comment on "A note on polarized light from Magnetars: QED effects and axion-like particles" by L.M. Capparelli, L. Maiani and A.D. Polosa

R. Turolla, S. Zane, R. Taverna +4

The recent detection of a large polarization degree in the optical emission of an isolated neutron star led to the suggestion that this has been the first evidence of vacuum polari…

astro-ph.SR2009★ 1 cited

The astrophysics of ultra-compact binaries

G. Nelemans, M. Wood, P. Groot +24

This white paper briefly describes the astrophysics of ultra-compact binaries, with emphasis of the challenges and opportunities in the next decade.

astro-ph2006★ 2 cited

Recent observational progress in AM CVn binaries

G. Ramsay, C. Brocksopp, P. Groot +9

We present the results of some recent research on AM CVn systems. We present: X-ray/UV observations made using XMM-Newton; the X-ray grating spectrum of RX J1914+24; preliminary re…

astro-ph2006★ 12 cited

A search for stellar X-ray sourcesin the Sagittarius and Carina dwarf galaxies - I: X-ray observations

G. Ramsay, K. Wu

ROSAT observations found no convincing evidence for X-ray sources located in local dwarf spheroidal galaxies (dSph). Now with more sensitive instruments on board Chandra and XMM-Ne…

astro-ph2004★ 4 cited

The Seyfert-LINER Galaxy NGC 7213: An XMM-Newton Observation

R. L. C. Starling, M. J. Page, G. Branduardi-Raymont +3

We examine the XMM X-ray spectrum of the LINER-AGN NGC 7213, which is best fit with a power law, K-alpha emission lines from Fe I, Fe XXV and Fe XXVI and a soft X-ray collisionally…