Next: The Objective Crystal Spectrometer
Up: Determining the Feasibility of
Previous: Simulating HEPC/LEPC Spectra
The total background per 2
diameter sperture in a
10
ksec observation is
likely to be
100 counts for LEPC and
30 counts
for HEPC. Therefore, Gaussian statistics can
be used to estimate the minimum count rate, Rmin, required to
detect a point
source at a given count rate significance, as a function of exposure
time T. For a point source on-axis, Rmin is given by the solution
to
or
Here,
is the signal-to-noise ratio of the net source
counts, expressed as number of
,
f is the encircled energy
fraction (0.5 on-axis), and RB is the total background rate in the
aperture. Results are shown in Figure 53 for
LEPC, and Figure 54 for HEPC, for a
range of background rates.
Figure 22:
HEPC/LEPC Effective Area.
The solid curve shows the effective area of one MM with the LEPC and
the dashed curve shows the effective area of one MM with the HEPC.
 |
Figure 23:
HEPC/LEPC Spatial Response.
For an 8 m focal length, 1 mm corresponds to
.
 |
Figure 24:
HEPC count rates yielding 1 ASCA SIS c s-1, for a power
law spectrum.
This and subsequent figures (25 - 50)
are
contour plots of count rate conversions derived from PIMMS.
 |
Figure 25:
HEPC count rates yielding 1 ASCA GIS c s-1, for a power
law spectrum.
 |
Figure 26:
HEPC count rates yielding 1 ROSAT PSPC c s-1, for a power
law spectrum.
 |
Figure 27:
HEPC count rates yielding 1 ASCA SIS c s-1, for a thermal
bremsstrahlung spectrum.
 |
Figure 28:
HEPC count rates yielding 1 ASCA GIS c s-1, for a thermal
bremsstrahlung spectrum.
 |
Figure 29:
HEPC count rates yielding 1 ROSAT PSPC c s-1, for a thermal
bremsstrahlung spectrum.
 |
Figure 30:
HEPC count rates yielding 1 ASCA SIS c s-1, for a blackbody
spectrum.
 |
Figure 31:
HEPC count rates yielding 1 ASCA GIS c s-1, for a blackbody
spectrum.
 |
Figure 32:
HEPC count rates yielding 1 ROSAT PSPC c s-1, for a blackbody
spectrum.
 |
Figure 33:
LEPC low-band count rates yielding 1 ASCA SIS c s-1, for a power
law spectrum.
This and subsequent figures (34 - 41)
are
contour plots of count rate conversions derived from PIMMS.
 |
Figure 34:
LEPC low-band count rates yielding 1 ASCA GIS c s-1, for a power
law spectrum.
 |
Figure 35:
LEPC low-band count rates yielding 1 ROSAT PSPC c s-1, for a power
law spectrum.
 |
Figure 36:
LEPC low-band count rates yielding 1 ASCA SIS c s-1, for a thermal
bremsstrahlung spectrum.
 |
Figure 37:
LEPC low-band count rates yielding 1 ASCA GIS c s-1, for a thermal
bremsstrahlung spectrum.
 |
Figure 38:
LEPC low-band count rates yielding 1 ROSAT PSPC c s-1, for a thermal
bremsstrahlung spectrum.
 |
Figure 39:
LEPC low-band count rates yielding 1 ASCA SIS c s-1, for a blackbody
spectrum.
 |
Figure 40:
LEPC low-band count rates yielding 1 ASCA GIS c s-1, for a blackbody
spectrum.
 |
Figure 41:
LEPC low-band count rates yielding 1 ROSAT PSPC c s-1, for a blackbody
spectrum.
 |
THIS PAGE INTENTIONALLY LEFT BLANK.
Figure 42:
LEPC high-band count rates yielding 1 ASCA SIS c s-1, for a power
law spectrum.
 |
Figure 43:
LEPC high-band count rates yielding 1 ASCA GIS c s-1, for a power
law spectrum.
 |
Figure 44:
LEPC high-band count rates yielding 1 ROSAT PSPC c s-1, for a power
law spectrum.
 |
Figure 45:
LEPC high-band count rates yielding 1 ASCA SIS c s-1, for a thermal
bremsstrahlung spectrum.
 |
Figure 46:
LEPC high-band count rates yielding 1 ASCA GIS c s-1, for a thermal
bremsstrahlung spectrum.
 |
Figure 47:
LEPC high-band count rates yielding 1 ROSAT PSPC c s-1, for a thermal
bremsstrahlung spectrum.
 |
Figure 48:
LEPC high-band count rates yielding 1 ASCA SIS c s-1, for a blackbody
spectrum.
 |
Figure 49:
LEPC high-band count rates yielding 1 ASCA GIS c s-1, for a blackbody
spectrum.
 |
Figure 50:
LEPC high-band count rates yielding 1 ROSAT PSPC c s-1, for a blackbody
spectrum.
 |
Figure 51:
LEPC pulse height spectrum simulated with XSPEC.
A 5 ksec LEPC observation of a Raymond-Smith plasma with cosmic
abundances, emission
integral of 1060 cm-3, temperature of 107.5 K, column
density of 1021 cm-2, and distance of 10 kpc is simulated.
 |
Figure 52:
HEPC pulse height spectrum simulated with XSPEC.
A 5 ksec HEPC observation of a Raymond-Smith plasma with cosmic
abundances, emission
integral of 1060 cm-3, temperature of 107.5 K, column
density of 1021 cm-2, and distance of 10 kpc is simulated.
 |
Figure 53:
Minimum Count Rate Detectable by LEPC.
The minimum count rate for a 5
count rate significance is
plotted as a function of exposure time, for 3 different background
rates (in c s-1) in a
diameter aperture on-axis,
using the formula given in
section 4.4.4.
 |
Figure 54:
Minimum Count Rate Detectable by HEPC.
The minimum count rate for a 5
count rate significance is
plotted as a function of exposure time, for 3 different background
rates (in c s-1) in a
diameter aperture on-axis,
using the formula given in
section 4.4.4.
 |
Next: The Objective Crystal Spectrometer
Up: Determining the Feasibility of
Previous: Simulating HEPC/LEPC Spectra
Tomas P. Girnius
1999-01-21