The GSFC MOXE Information Page


The MOnitoring X-ray Experiment (MOXE)
is an X-ray all-sky monitor
to be launched on the Russian Spectrum-X-Gamma satellite. It will
monitor several hundred X-ray sources on a daily basis, and due to
its four day high-earth orbit will be the
first instrument to monitor most of the X-ray sky most of the time. MOXE
will serve as an alarm, to alert users of more
sensitive instruments on Russia's giant high
energy astrophysics observatory and of other instruments to transient
activity. MOXE will also produce long time baseline light curves of many
sources which will be virtually free of gaps due to Earth occultation.
MOXE consists of an array of 6 X-ray pinhole detectors,
sensitive from 2 to 25 keV, which views 4 pi steradians (except for a
20 X 80 square degree patch which obscures the Sun). The pinhole
apertures of 0.625 X 2.556 square cm imply an angular resolution of 2.4
X 9.7 square degrees(FWHM on-axis).
The flight instrument will mass
approximately 118 kg and draw 38 Watts. For a non-focussing all-sky
instrument that is limited by sky background, the limiting sensitivity
is a function only of detector area. MOXE will, for a 24 hrs exposure,
have a sensitivity of approximately 2 mCrab. MOXE distinguishes itself
with respect to other all-sky monitors in its high duty cycle, thus
having unprecendented sensitivity to transient phenomena with time
scales between minutes and hours.


above is a simulation of a MOXE data product: an X-ray sky map.
The image is displayed in galactic coordinates. Bright
sources along the galactic plane are shown in red; the distortion is due to
the non-circular detector aperture. Dark blue lines are areas of detector
overlap, where more than one detector is imaging the same area of the sky.
The lighter green lines are an artifact of the detector structure. Black
patches are due to areas on three detectors which block out the strong signal
from the Sun.
History
Calibration Images: in progress!
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