83 citations · 252 across the 10 of their papers we have counts for
10 papers
Revolutionary Solar System Science Enabled by the Line Emission Mapper X-ray Probe
William R. Dunn, Dimitra Koutroumpa, Jennifer A. Carter +27
The Line Emission Mapper's (LEM's) exquisite spectral resolution and effective area will open new research domains in Astrophysics, Planetary Science and Heliophysics. LEM will pro…
Exploring Fundamental Particle Acceleration and Loss Processes in Heliophysics through an Orbiting X-ray Instrument in the Jovian System
W. Dunn, G. Berland, E. Roussos +41
Jupiter's magnetosphere is considered to be the most powerful particle accelerator in the Solar System, accelerating electrons from eV to 70 MeV and ions to GeV energies. How elect…
Photoionisation Modelling of the X-ray Emission Line Regions within the Seyfert 2 AGN NGC 1068
S. Grafton-Waters, G. Branduardi-Raymont, M. Mehdipour +4
We investigate the photoionised X-ray emission line regions (ELRs) within the Seyfert 2 galaxy NGC 1068, to determine if there are any characteristic changes between observations t…
The in-situ exploration of Jupiter's radiation belts (A White Paper submitted in response to ESA's Voyage 2050 Call)
Elias Roussos, Oliver Allanson, Nicolas André +26
Jupiter has the most energetic and complex radiation belts in our solar system. Their hazardous environment is the reason why so many spacecraft avoid rather than investigate them,…
Anatomy of the AGN in NGC 5548 IX. Photoionized emission features in the soft X-ray spectra
Junjie Mao, J. S. Kaastra, M. Mehdipour +10
The X-ray narrow emission line region (NELR) of the archetypal Seyfert 1 galaxy NGC\,5548 has been interpreted as a single-phase photoionized plasma that is absorbed by some of the…
The Filter Wheel and Filters development for the X-IFU instrument on-board Athena
E. Bozzo, M. Barbera, L. Genolet +7
Athena is the large mission selected by ESA in 2013 to investigate the science theme "Hot and Energetic Universe" and presently scheduled for launch in 2028. One of the two instrum…
X-rays from Saturn: A study with XMM-Newton and Chandra over the years 2002-05
G. Branduardi-Raymont, A. Bhardwaj, R. F. Elsner +1
We present the results of the two most recent (2005) XMM-Newton observations of Saturn together with the re-analysis of an earlier (2002) observation from the XMM-Newton archive an…
XMM-Newton observations of X-ray emission from Jupiter
G. Branduardi-Raymont, A. Bhardwaj, R. F. Elsner +6
We present the results of two XMM-Newton observations of Jupiter carried out in 2003 for 100 and 250 ks (or 3 and 7 planet rotations) respectively. X-ray images from the EPIC CCD c…
Solar Control on Jupiter's Equatorial X-ray Emissions: 26-29 November 2003 XMM-Newton Observation
Anil Bhardwaj, Graziella Branduardi-Raymont, Ronald F. Elsner +6
During November 26-29, 2003 XMM-Newton observed soft (0.2-2 keV) X-ray emission from Jupiter for 69 hours. The low-latitude X-ray disk emission of Jupiter is observed to be almost…
Can a Dusty Warm Absorber Model Reproduce the Soft X-ray Spectra of MCG-6-30-15 and Mrk 766?
M. Sako, S. M. Kahn, G. Branduardi-Raymont +8
XMM-Newton RGS spectra of MCG-6-30-15 and Mrk 766 exhibit complex discrete structure, which was interpreted in a paper by Branduardi-Raymont et al. (2001) as evidence for the exist…