FOC Exposure Simulator - FOCSIM
The FOC Exposure Simulator, FOCSIM, provides the capability to simulate
almost any FOC exposure and to calculate diagnostics about the image.
FOCSIM, the FOC exposure SIMulator, uses the most current description
of the FOC and its filters along with an input spectra (either from an
on-line catalog or user-supplied file) to simulate an image from the
FOC and provide the count rate within the image. FOCSIM provides not
only a calculation of the exposure time needed to reach a desired S/N,
but also statistics related to the count rate that is expected from the
object and how it is spread across a spherically-aberrated source or
across a COSTAR-corrected source.
FOCSIM
The WWW form
allows you to run FOCSIM to simulate a 512x512 FOC image
of an individual point-source, without creating the actual image.
The results of each simulation are returned as a page which can be
saved if desired.
How to run FOCSIM
The FOCSIM Beginner's Manual
walks the user through their first FOCSIM session, step-by-step, then
discusses more advanced uses of FOCSIM, including using user-supplied
spectra.
How FOCSIM Works
FOCSIM starts with a given spectrum for the source and calculates the
count rate based on the equations given in the FOC Handbook. Similarly,
the count rates for the background sources the user specifies are
calculated based on the equations in the FOC Handbook. For a point
source, however, the count rate distribution over the detector area is
specified by the Point Spread Function (PSF). There are two libraries
of PSFs available to FOCSIM, one of theoretical mono-chromatic PSFs and
one of observed PSFs. For the COSTAR-corrected FOC, a set of
theoretical PSFs have been created based on the best descriptions
available of COSTAR and the FOC. FOCSIM then utilizes files for the camera
DQE based on in-flight calibration observations, a table with the
measured reflectivities for the COSTAR FOC mirrors (for use in
COSTAR-corrected FOC simu-lations), a library of measured filter
throughputs kept in the Calibration Database System (CDBS), and files
for the OTA's throughput taken from CDBS as well. This ensures the
users of FOCSIM that the latest calibration data available has been
incorporated into the simulation to provide as accurate a description
of the FOC as possible.
What Sources can FOCSIM Simulate
There are three libraries of spectra available to FOCSIM: BPGS spectra, UCB
spectra and CLB spectra. The BPGS spectra are observed spectra for many stellar
standards used in astronomy, while the CLB spectra are spectra for objects used
for calibrating the HST instruments. The UCB spectra are theoretical stellar
spectra for over 75 MK classes. These provide a base for simulating a wide range
of stellar observations, however not all observations are of stellar objects. FOCSIM
also has the capability to create its own synthetic spectra using either power-law,
black-body, or flat spectral models, normalized to whatever parameters the user
gives. Finally, the user can supply their own spectra for the most accurate simulation,
if it is available. These choices allows the user to examine almost any object
as if viewed through the FOC.
What FOCSIM Calculates
The output from FOCSIM can include an image, several STSDAS tables and
output report of the calculations. In general the most significant
results are included in the standard output report, similar to:
Computed energy_fraction 0.6947
Exposure time: 183.9 [Seconds]
ST MAG 22.75
Source area for min exposure time 81.00 [Pixels]
Source rate in Source area 0.6283 [Counts s-1]
Total backg Rate 0.4883E-01
TOTAL SOURCE RATE 0.9044
Rates in the Point Source Center Pixel:
Point Source Rate 0.7153E-01 [Counts pixel-1 s-1]
Using these results, a potential observer can determine whether or not his
source object would suffer from any linearity or saturation problems and adjust the
filters used accordingly.
Where do I go if something doesn't look or work right?
All materials for FOCSIM have been written by the STScI FOC group.
Questions about running FOCSIM or about what FOCSIM can do for you can
be directed through the STScI Help Desk.
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