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- J. Osborne4 profiles56 · h 67
- U. Leicester41 · h 43
- K. Page3 profiles39 · h 57
- N. Tanvir3 profiles38 · h 81
- A. Levan2 profiles32 · h 74
- P. O’Brien3 profiles29 · h 74
- D. Burrows2 profiles28 · h 57
- T. Lister2 profiles28 · h 44
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- N. Gehrels4 profiles27 · h 120
- P. Romano4 profiles26 · h 49
- M. Watson3 profiles25 · h 39
- Goddard Space Flight CenterUS68 papers
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35 papers · 1 filter
Detecting emission lines with XMM-Newton in 4U 1538-52
J. J. Rodes-Roca, K. L. Page, J. M. Torrejón +2
Context. The properties of the X-ray emission lines are a fundamental tool for studying the nature of the matter surrounding the neutron star and the phenomena that produce these l…
Confirmation of the Supergiant Fast X-ray Transient nature of AX J1841.0-0536 from Swift outburst observations
P. Romano, V. Mangano, G. Cusumano +8
Swift observed an outburst from the supergiant fast X-ray transients (SFXT) AX J1841.0-0536 on 2010 June 5, and followed it with XRT for 11 days. The X-ray light curve shows an ini…
p, He, and C to Fe cosmic-ray primary fluxes in diffusion models: Source and transport signatures on fluxes and ratios
A. Putze, D. Maurin, F. Donato
The propagated fluxes of proton, helium, and heavier primary cosmic-ray species (up to Fe) are a means to indirectly access the source spectrum of cosmic rays. We check the compati…
The Super-Soft X-ray Phase of Nova RS Ophiuchi 2006
J. P. Osborne, K. L. Page, A. P. Beardmore +13
Swift X-ray observations of the ~60 day super-soft phase of the recurrent nova RS Ophiuchi 2006 show the progress of nuclear burning on the white dwarf in exquisite detail. First s…
X-ray spectral state is not correlated with luminosity in Holmberg II X-1
Fabien Grisé, Philip Kaaret, Hua Feng +2
The ultraluminous X-ray source (ULX) Holmberg II X-1 has been observed over 4 months in 2009/2010 by the Swift observatory. The source luminosity varied by a factor of up to 14, re…
Assumptions of IV Methods for Observational Epidemiology
Vanessa Didelez, Sha Meng, Nuala A. Sheehan
Instrumental variable (IV) methods are becoming increasingly popular as they seem to offer the only viable way to overcome the problem of unobserved confounding in observational st…