18 research outputs found
A setup for soft proton irradiation of X-ray detectors for future astronomical space missions
Protons that are trapped in the Earth's magnetic field are one of the main
threats to astronomical X-ray observatories. Soft protons, in the range from
tens of keV up to a few MeV, impinging on silicon X-ray detectors can lead to a
significant degradation of the detector performance. Especially in low earth
orbits an enhancement of the soft proton flux has been found. A setup to
irradiate detectors with soft protons has been constructed at the Van-de-Graaff
accelerator of the Physikalisches Institut of the University of T\"ubingen. Key
advantages are a high flux uniformity over a large area, to enable irradiations
of large detectors, and a monitoring system for the applied fluence, the beam
uniformity, and the spectrum, that allows testing of detector prototypes in
early development phases, when readout electronics are not yet available. Two
irradiation campaigns have been performed so far with this setup. The
irradiated detectors are silicon drift detectors, designated for the use
on-board the LOFT space mission. This paper gives a description of the
experimental setup and the associated monitoring system.Comment: 20 pages, 10 figures, 4 table
XMM-EPIC observation of MCG-6-30-15: Direct evidence for the extraction of energy from aspinning black hole?
We present XMM-Newton European Photon Imaging Camera (EPIC) observations of
the bright Seyfert 1 galaxy MCG-6-30-15, focusing on the broad Fe K
line at ~6keV and the associated reflection continuum, which is believed to
originate from the inner accretion disk. We find these reflection features to
be extremely broad and red-shifted, indicating its origin from the very most
central regions of the accretion disk. It seems likely that we have caught this
source in the ``deep minimum'' state first observed by Iwasawa et al. (1996).
The implied central concentration of X-ray illumination is difficult to
understand in any pure accretion disk model. We suggest that we are witnessing
the extraction and dissipation of rotational energy from a spinning black hole
by magnetic fields connecting the black hole or plunging region to the disk.Comment: 6 pages and one postscript figure. Accepted for publication in MNRAS
letter
Improving XMM-Newton EPIC pn data at low energies: method and application to the Vela SNR
High quantum efficiency over a broad spectral range is one of the main
properties of the EPIC pn camera on-board XMM-Newton. The quantum efficiency
rises from ~75% at 0.2 keV to ~100% at 1 keV, stays close to 100% until 8 keV,
and is still ~90% at 10 keV. The EPIC pn camera is attached to an X-ray
telescope which has the highest collecting area currently available, in
particular at low energies (more than 1400 cm2 between 0.1 and 2.0 keV). Thus,
this instrument is very sensitive to the low-energy X-ray emission. However,
X-ray data at energies below ~0.2 keV are considerably affected by detector
effects, which become more and more important towards the lowest transmitted
energies. In addition to that, pixels which have received incorrect offsets
during the calculation of the offset map at the beginning of each observation,
show up as bright patches in low-energy images. Here we describe a method which
is not only capable of suppressing the contaminations found at low energies,
but which also improves the data quality throughout the whole EPIC pn spectral
range. This method is then applied to data from the Vela supernova remnant.Comment: Proc. SPIE Vol. 5488: Astronomical Telescopes and Instrumentation, UV
- Gamma-Ray Space Telescope Systems, Eds. Guenther Hasinger and Martin J.
Turner, 22-24 June 2004, Glasgow, Scotland United Kingdo
On the deep minimum state in the Seyfert galaxy MCG-6-30-15
(abridged) We present a detailed spectral analysis of the first observation
of the Seyfert 1 galaxy MCG-6-30-15 by the European Photon Imaging Camera on
board the XMM-Newton observatory, together with contemporaneous data from the
Proportional Counter Array on the Rossi X-ray Timing Explorer. Confirming our
previously published result, we find that the presence of extremely broadened
reflection features from an ionized relativistic accretion disk is required
even when one employs the latest X-ray reflection models and includes the
effect of complex absorption. The extremely broadened reflection features are
also present if the primary continuum is modeled with a thermal Comptonisation
spectrum rather than a simple power-law continuum. With this fact established,
we examine these data using a relativistic smearing function corresponding to a
``generalized thin accretion disk'' model. We find strong evidence for torquing
of the central parts of the accretion disk (presumably through magnetic
interactions with the plunging region of the disk and/or the rotating black
hole itself). We also perform a study of spectral variability within our
observation. We find that the disk reflection features maintain roughly a
constant equivalent width with respect to the observed continuum, as predicted
by simple reflection models. Taken together with other studies of MCG-6-30-15
that find disk features to possess constant intensity at higher flux states, we
suggest that the flux of disk features undergoes a saturation once the source
emerges from a Deep Minimum state.Comment: 16 pages, accepted for publication in MNRA