The performance and characteristics of the flight PSPCs were measured extensively. Here
we present some results on their energy and position response measured with 8 keV
X-rays collimated to 150 m radius at an applied anode voltage of 1700 V. The
collimated X-rays were projected on
grid points at 0.94 mm intervals on
PSPC aperture. It has been noticed at the previous calibration of WXM/HETE-1
(Yamauchi et al. 1997;
Tokanai 1997)
that the self-induced space charge effect degrades energy resolution
and its linearity at high anode voltages. In the HETE-2 counters, the energy
resolution becomes worse at
V while the position resolution gradually
improves at higher voltages and reaches 0.6 mm (FWHM) around 1700 V. Therefore we
choose to operate around 1650 V in order to achieve good position resolution
of <1 mm, which is required for PSPC/WXM to
localize GRBs with 10
accuracy in 2-second integration time. Here we present
some results from a counter at 1700 V anode voltage.
The linearity of the output pulse height (sum of the charges collected at the left and
right ends) to the incidence photon energy was measured for one PSPC using
monochromatic X-ray beams with energies 6-24 keV with 2 keV step. While at the
applied voltage of 1400 V there is a good linearity between them, at 1700 V the
linearity is not conserved due to the self-induced space charge effect. The energy
resolution is mostly uniform (22% at 8.04 keV with 1700 V anode voltage) except near
the wire ends ( mm) where the electric field is distorted by the wall of the
counter.
The position of an incident X-ray is determined from X = L / (L + R), the
ratio of the charge collected at the left and right ends of the anode wire. Ideally the
ratio X is expected to have a linear relation with the incident position x along
the anode. In reality there is nonlinearity near the ends of anode wire
(Fig. 2). We use an empirical analytical formula to calculate the
incident position from the measured charge ratio X. The parameters of
the formula are determined for each anode wire by fitting the measured curve. The
position resolution was also found to be mostly uniform at 0.6-0.7 mm except near
the wire ends. In Fig. 3 the position resolution expressed by the
FWHM of the distribution of
is plotted against incident position x.
Copyright The European Southern Observatory (ESO)