1,988 research outputs found
High-Resolution spectroscopy of the low-mass X-ray binary EXO 0748-67
We present initial results from observations of the low-mass X-ray binary EXO
0748-67 with the Reflection Grating Spectrometer on board the XMM-Newton
Observatory. The spectra exhibit discrete structure due to absorption and
emission from ionized neon, oxygen, and nitrogen. We use the quantitative
constraints imposed by the spectral features to develop an empirical model of
the circumsource material. This consists of a thickened accretion disk with
emission and absorption in the plasma orbiting high above the binary plane.
This model presents challenges to current theories of accretion in X-ray binary
systems.Comment: 5 pages, 4 figures, accepted by A&A letters, XMM special issu
KASR: A Reliable and Practical Approach to Attack Surface Reduction of Commodity OS Kernels
Commodity OS kernels have broad attack surfaces due to the large code base
and the numerous features such as device drivers. For a real-world use case
(e.g., an Apache Server), many kernel services are unused and only a small
amount of kernel code is used. Within the used code, a certain part is invoked
only at runtime while the rest are executed at startup and/or shutdown phases
in the kernel's lifetime run. In this paper, we propose a reliable and
practical system, named KASR, which transparently reduces attack surfaces of
commodity OS kernels at runtime without requiring their source code. The KASR
system, residing in a trusted hypervisor, achieves the attack surface reduction
through a two-step approach: (1) reliably depriving unused code of executable
permissions, and (2) transparently segmenting used code and selectively
activating them. We implement a prototype of KASR on Xen-4.8.2 hypervisor and
evaluate its security effectiveness on Linux kernel-4.4.0-87-generic. Our
evaluation shows that KASR reduces the kernel attack surface by 64% and trims
off 40% of CVE vulnerabilities. Besides, KASR successfully detects and blocks
all 6 real-world kernel rootkits. We measure its performance overhead with
three benchmark tools (i.e., SPECINT, httperf and bonnie++). The experimental
results indicate that KASR imposes less than 1% performance overhead (compared
to an unmodified Xen hypervisor) on all the benchmarks.Comment: The work has been accepted at the 21st International Symposium on
Research in Attacks, Intrusions, and Defenses 201
The interstellar oxygen-K absorption edge as observed by XMM-Newton
High resolution X-ray spectra of the Reflection Grating Spectrometer (RGS) on
board the XMM satellite are used to resolve the oxygen K absorption edge. By
combining spectra of low and high extinction sources, the observed absorption
edge can be split in the true interstellar (ISM) extinction and the
instrumental absorption. The detailed ISM edge structure closely follows the
edge structure of neutral oxygen as derived by theoretical R-matrix
calculations. However, the position of the theoretical edge requires a
wavelength shift. In addition the detailed instrumental RGS absorption edge
structure is presented. All results are verified by comparing to a subset of
Chandra LETG-HRC observations.Comment: LaTeX2e A&A style, 10 pages, 12 postscript figures, accepted for
publication in Astronomy and Astrophysic
Optimizing the Data Available Via Health Canada\u27s Clinical Information Portal
Through its Public Release of Clinical Information initiative, Health Canada has provided public access to a vast repository of data that have been submitted to support market authorization of drugs and medical devices. Health Canada has released data from more than 160 submissions for drugs, biologics, vaccines and medical devices. The regulator is currently in its third year of a 4-year phase-in schedule to release clinical data proactively from submissions for all new active substances, new clinical indications, generic drugs and higher-risk devices that are approved, withdrawn or rejected. Substantial clinical data submitted by the industry sponsor of the application, including summary-level data and metadata are made publicly available by Health Canada as a matter of policy
A New Comprehensive 2-D Model of the Point Spread Functions of the XMM-Newton EPIC Telescopes : Spurious Source Suppression and Improved Positional Accuracy
We describe here a new full 2-D parameterization of the PSFs of the three
XMM-Newton EPIC telescopes as a function of instrument, energy, off-axis angle
and azimuthal angle, covering the whole field-of-view of the three EPIC
detectors. It models the general PSF envelopes, the primary and secondary
spokes, their radial dependencies, and the large-scale azimuthal variations.
This PSF model has been constructed via the stacking and centering of a large
number of bright, but not significantly piled-up point sources from the full
field-of-view of each EPIC detector, and azimuthally filtering the resultant
PSF envelopes to form the spoke structures and the gross azimuthal shapes
observed. This PSF model is available for use within the XMM-Newton Science
Analysis System via the usage of Current Calibration Files XRTi_XPSF_0011.CCF
and later versions. Initial source-searching tests showed substantial
reductions in the numbers of spurious sources being detected in the wings of
bright point sources. Furthermore, we have uncovered a systematic error in the
previous PSF system, affecting the entire mission to date, whereby returned
source RA and Dec values are seen to vary sinusoidally about the true position
(amplitude ~0.8") with source azimuthal position. The new PSF system is now
available and is seen as a major improvement with regard to the detection of
spurious sources. The new PSF also largely removes the discovered astrometry
error and is seen to improve the positional accuracy of EPIC. The modular
nature of the PSF system allows for further refinements in the future.Comment: Accepted for publication in A&A. 15 pages, 13 figures (some of
reduced quality). A full-resolution version is available at
http://www.star.le.ac.uk/~amr30/amr_PSFpaper.pd
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras
The second XMM-Newton serendipitous source catalogue, 2XMM, provides the
ideal data base for performing a statistical evaluation of the flux
cross-calibration of the XMM-Newton European Photon Imaging Cameras (EPIC). We
aim to evaluate the status of the relative flux calibration of the EPIC cameras
on board XMM-Newton (MOS1, MOS2, and pn) and investigate the dependence of the
calibration on energy, position in the field of view of the X-ray detectors,
and lifetime of the mission. We compiled the distribution of flux percentage
differences for large samples of 'good quality' objects detected with at least
two of the EPIC cameras. The mean offset of the fluxes and dispersion of the
distributions was then found by Gaussian fitting. Count rate to flux conversion
was performed with a fixed spectral model. The impact on the results of varying
this model was investigated. Excellent agreement was found between the two EPIC
MOS cameras to better than 4% from 0.2 keV to 12.0 keV. MOS cameras register
7-9% higher flux than pn below 4.5 keV and 10-13% flux excess above 4.5 keV. No
evolution of the flux ratios is seen with time, except at energies below 0.5
keV, where we found a strong decrease in the MOS to pn flux ratio with time.
This effect is known to be due to a gradually degrading MOS redistribution
function. The flux ratios show some dependence on distance from the optical
axis in the sense that the MOS to pn flux excess increases with off-axis angle.
Furthermore, in the 4.5-12.0 keV band there is a strong dependence of the MOS
to pn excess flux on the azimuthal-angle. These results strongly suggest that
the calibration of the Reflection Grating Array (RGA) blocking factors is
incorrect at high energies. Finally, we recommend ways to improve the
calculation of fluxes in future versions of XMM-Newton source catalogues.Comment: 11 pages, 10 figures, 3 tables. Abridged Abstract. Accepted for
publication in Astronomy and Astrophysic
High Resolution X-ray Spectroscopy of G292.0+1.8/MSH 11-54
We present a preliminary analysis of XMM-Newton observations of the
oxygen-rich supernova remnant G292.0+1.8 (MSH 11-54). Although the spatial
extent of the remnant is 8 arcmin the bright central bar is narrow (1'-2')
resulting in RGS spectra of a high spectral quality. This allows us to
spectroscopically identify a cool, Te = 0.3 keV, and underionized component,
resolve details of the Fe-L complex, and resolve the forbidden and resonant
lines of the O VII triplet. We are also able to constrain the kinematics of the
remnant using Ne IX as observed in the second order spectrum, and O VIII in the
first order spectrum. We do not find evidence for O VII line shifts or Doppler
broadening (sigma_v < 731 km/s), but line broadening of the Ne X Ly-alpha line
seems to be present, corresponding to sigma_v ~ 1500 km/s.Comment: To appear in Proc. of the BeppoSAX Symposium: "The Restless
High-Energy Universe", E.P.J. van den Heuvel, J.J.M. in 't Zand, and R.A.M.J.
Wijers (Eds
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