Parameter | Mand | Type | Default | Constraints |
smoothingcounts | yes | int | 50 | |
The number of counts to accumulate for the smoothing
| ||||
thresholdmasking | yes | real | 0.02 | |
The scale factor for excluding regions from the smoothing based on a mask image.
In the default mode the average exposure is calculated and then any pixel with
exposure less than fraction*average value is excluded.
| ||||
detector | yes | int | 0|1 | |
Detector, 1 for a specific instrument and exposure, 0 for the
combined image (i.e., the output of comb). | ||||
elow | yes | int | 400 | |
The low energy for the band in eV
| ||||
ehigh | yes | int | 1250 | |
The high energy for the band in eV
| ||||
binning | yes | int | 1 | |
Binning control with 1 for no binning, and integers greater than 1 for
binning that number of pixels in each dimension.
| ||||
withpartcontrol | yes | bool | yes | |
Particle background control, "yes" to subtract the model particle background image.
| ||||
withsoftcontrol | yes | bool | no | |
Soft proton background control, "yes" to subtract the soft proton background image.
| ||||
withswcxcontrol | yes | bool | no | |
Solar wind charge exchange background control, "yes" to subtract the SWCX background image.
| ||||
withmaskcontrol | yes | bool | no | |
Control for including an additional masking image.
| ||||
maskfile | yes | dataset | ||
The file name for an image to provide additional masking if desired.
If left blank then there will be no additional masking.
The mask images must be the same size and projection as the other images.
| ||||
prefix | yes | string | 1S001 | |
Prefix defining the exposure used, with the esas nomenclature, eg.
S003 means PN S003 exposure, while 1S002 and 2S003 mean MOS1 S002 and MOS2
S003 exposures, respectively.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
smoothingcounts | yes | int | 100 | |
The number of counts to accumulate for the smoothing
| ||||
thresholdmasking | yes | real | 0.02 | |
The scale factor for excluding regions from the smoothing based on a mask
image. In the default mode the average exposure is calculated and then
any pixel with exposure less than fraction*average value is excluded.
| ||||
elowlist | yes | int | 400 750 | |
Low energy for successive bands in eV
| ||||
ehighlist | yes | int | 750 1250 | |
High energy for successive bands in eV
| ||||
binning | yes | int | 1 | |
Binning control, number of pixels (in both dimensions) to be binned.
| ||||
withpartcontrol | yes | bool | yes | |
Particle background control, "yes" to subtract the model particle background image.
| ||||
withsoftcontrol | yes | bool | no | |
Soft proton background control, "yes" to subtract the soft proton background image.
| ||||
withswcxcontrol | yes | bool | no | |
Solar wind charge exchange background control, "yes" to subtract the SWCX
background image.
| ||||
withoffsetbkgcontrol | yes | bool | yes | |
Offset background control, "yes" to subtract the offset background image.
This is a feature currently under development and is not yet functional.
| ||||
withmaskcontrol | yes | bool | yes | |
Mask control, "yes" for using a mask image (pixel with 1 in image will be
included, pixel with 0 will be excluded).
| ||||
mask | yes | dataset | mask.fit | |
Mask image file name.
| ||||
fill | yes | int | 1 | |
Number of passes to fill in empty pixels. If a zero pixel has three or more
non-zero neighbors, the pixel will be the average value of those neighbors.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
thresholdmasking | yes | real | 0.02 | |
The scale factor for excluding regions from the smoothing based on a mask
image. In the default mode the average exposure is calculated and then
any pixel with exposure less than fraction*average value is excluded.
| ||||
detector | yes | int | ||
Detector selection, 0: combined exposures, 1: MOS, 2: PN.
| ||||
prefix | yes | string | 1S001 | |
Prefix defining the exposure used, with the esas nomenclature, eg.
S003 means PN S003 exposure, while 1S002 and 2S003 mean MOS1 S002 and MOS2
S003 exposures, respectively.
| ||||
elow | yes | int | 400 | |
Low energy for band in eV
| ||||
ehigh | yes | int | 1250 | |
High energy for band in eV
| ||||
binning | yes | int | 1 | |
Binning control with 1 for no binning, other integers for binning.
| ||||
withpartcontrol | yes | bool | yes | |
Particle background control, "yes" to subtract the model particle background image.
| ||||
withsoftcontrol | yes | bool | no | |
Soft proton background control, "yes" to subtract the soft proton background image.
| ||||
withswcxcontrol | yes | bool | no | |
Solar wind charge exchange background control, "yes" to subtract the
SWCX background image.
| ||||
withmaskcontrol | yes | bool | no | |
Solar wind charge exchange background control, "yes" to subtract the
SWCX background image.
| ||||
mask | yes | dataset | mask.fit | |
Mask image file name (defaults to using exposure mask).
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
thresholdmasking | yes | real | 0.02 | |
The scale factor for excluding regions from the smoothing based on a mask image.
In the default mode the average exposure is calculated and then any pixel with
exposure less than fraction*average value is excluded.
| ||||
elowlist | yes | int | 350 800 | |
Low energy for successive bands in eV
| ||||
ehighlist | yes | int | 800 1300 | |
High energy for successive bands in eV
| ||||
binning | yes | int | 1 | |
Binning control with 1 for no binning, 2,4,8,16,32 for binning by 2,
4,8,16,32.
| ||||
withpartcontrol | yes | bool | yes | |
Particle background control, "yes" to subtract the model particle background image.
| ||||
withsoftcontrol | yes | bool | yes | |
Soft proton background control, "yes" to subtract the soft proton background image.
| ||||
withswcxcontrol | yes | bool | yes | |
Solar wind charge exchange background control, "yes" to subtract the swcx background image.
| ||||
withmaskcontrol | yes | bool | yes | |
For masking with an additional image.
| ||||
mask | yes | dataset | mask.fit | |
Mask image file name.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
prefixm | yes | string | ||
Detector and exposure identifiers (eg. "1S001 2S002") for the MOS exposures
(in the example MOS1 S001 and MOS2 S002) to be processed.
| ||||
prefixp | yes | string | ||
Detector and exposure identifiers (eg. "S003") for the PN exposures
(in the example PN S003) to be processed.
| ||||
verb | yes | int | 4 | |
SAS verbosity level.
| ||||
scale | yes | real | 0.5 | |
Energy fraction, which sets the exclusion radius of point sources.
| ||||
rate | yes | real | 1.0 | |
Flux threshold (in units of ![]() | ||||
dist | yes | real | ||
Minimum separation in arc seconds between masked sources.
| ||||
elow | yes | int | 400 | |
The low energy for the band in eV
| ||||
ehigh | yes | int | 1250 | |
The high energy for the band in eV
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
prefixm | yes | string | ||
Detector and exposure identifiers (eg. "1S001 2S002") for the MOS exposures
(in the example MOS1 S001 and MOS2 S002) to be processed.
| ||||
prefixp | yes | string | ||
Detector and exposure identifiers (eg. "S003") for the PN exposures
(in the example PN S003) to be processed.
| ||||
verb | yes | int | 4 | |
SAS verbosity level.
| ||||
scale | yes | real | 0.5 | |
Energy fraction, which sets the exclusion radius of point sources.
| ||||
ratet | no | real | 1.0 | |
Total flux threshold for exclusion of pt srcs
| ||||
rates | no | real | 1.0 | |
Soft flux threshold for exclusion of pt srcs
| ||||
rateh | no | real | 1.0 | |
Hard flux threshold for exclusion of pt srcs
| ||||
dist | no | real | ||
Minimum separation in arc seconds between masked sources
| ||||
elowlist | yes | int | 400 2000 | |
Lower energy limit list for the energy bands in eV
| ||||
ehighlist | yes | int | 1300 7200 | |
Higher energy limit list for the energy bands in eV
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
caldb | yes | string | ||
Directory containing all the ESAS specific calibration files
| ||||
withpartcontrol | yes | boolean | true | |
Particle background flag, 'true' to include it.
| ||||
withsoftcontrol | yes | boolean | true | |
Soft proton background flag, 'true' to include it.
| ||||
withswcxcontrol | yes | boolean | true | |
SWCX background flag, 'true' to include it.
| ||||
alpha | yes | real | 1.7 | |
Assumed spectral index for the filter correction scaling.
| ||||
elowlist | yes | int | 400 750 | |
Energy low limit(s) (in eV) for the different bands.
| ||||
ehighlist | yes | int | 750 1250 | |
Energy high limit(s) (in eV) for the different bands.
| ||||
mask | yes | int | ||
Masking control. 0: No additional masking,
1: uses the mask produced by the cheese task, 2: uses the
normal mask images produced by eexpmap, and 3: uses the normal mask
images produced by eexpmap modified by make-mask.
| ||||
prefixlist | yes | string | 1S001 2S002 S003 | |
Exposure identifiers (eg. "1S001 2S002 S003") for the exposures
(in the example MOS1 S001, MOS2 2S002, and PN S003) to be processed.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
detector | yes | string | ||
The instrument identifier (EMOS1, EMOS2, or PN).
| ||||
mode | yes | int | ||
conv_reg operational mode:
mode=1 - region fits files are both input and output mode=2 - ascii files with region parameters are both input and output mode=3 - command line input of individual region parameters and screen output | ||||
imagefile | yes | string | ||
Filename image in sky coordinates - used to extract observation position angle.
| ||||
ra | no | real | none | |
mode=3 RA input | ||||
dec | no | real | none | |
mode=3 Dec input | ||||
shape | no | real | none | |
mode=3 region shape input, only circle and ellipse
at this time (either all upper or all lower case, along with their ``nots'',
e.g., ``!ELLIPSE'') | ||||
radius | no | real | none | |
mode=3 radius for circular region input | ||||
semimajor | no | real | none | |
mode=3 semimajor axis (in arc minutes) for
elliptical region input | ||||
semiminor | no | real | none | |
mode=3 semiminor axis (in arc minutes) for
elliptical region input | ||||
rotangle | no | real | none | |
mode=3 rotation angle (in degrees) for
elliptical region input | ||||
inputfile | no | string | ||
mode=1,2 input file name | ||||
outputfile | no | string | ||
mode=1,2 input file name | ||||
sublist | yes | string | mosaic-times.txt | |
Ascii file with the output of esprep_mosaic_times
| ||||
m1prefix | yes | string | 1S001 | |
MOS1 ESAS prefix
| ||||
m2prefix | yes | string | 2S002 | |
MOS2 ESAS prefix
| ||||
pnprefix | yes | string | S003 | |
PN ESAS prefix
| ||||
eventset | no | string | none | |
list of event files | ||||
method | no | string | corner | |
which method to use. | ||||
withsmoothing | no | boolean | N | Y/N |
Smooth data? | ||||
smooth | no | integer | 50 | ![]() |
Smoothing factor in seconds | ||||
withbinning | no | boolean | N | Y/N |
Bin data? | ||||
binning | no | integer | 50 | ![]() |
Bin width in seconds | ||||
withspecranges | no | boolean | N | Y/N |
Use upper/lower spec chans? | ||||
specchanmin | no | integer | 2500 | ![]() ![]() |
Low Spectral Channel | ||||
specchanmax | no | integer | 12000 | ![]() ![]() |
High Spectral Channel | ||||
ratio | no | real | 1.2 | ![]() ![]() |
Flaring ratio of annulus_cnts corn_area corn_cnst annu_area | ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
eventsin | yes | string | mos1S001-clean_P001.ds | |
Input event list from emosaic_prep.
| ||||
eventsout | yes | string | mos1S001-clean.fits | |
Output event list for use with ESAS.
| ||||
raobj | yes | real | 270.0 | |
Reference RA of the sub-pointing.
| ||||
decobj | yes | real | 45.0 | |
Reference Dec of the sub-pointing.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
atsfile | yes | string | ||
Input ODF *ATS.FIT file.
| ||||
sasfile | yes | string | ||
Input summary ODF *SUM.SAS file created by odfingest.
| ||||
inimage | no | string | inimage.fit | |
Event image for the exposure
| ||||
inmask | no | string | inmask.fit | |
Exposure mask
| ||||
outmask | no | string | outmask.fit | |
The output file name for the cheese mask
| ||||
reglist | no | string | reglist.fit | |
The filtered source region list.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
srclist | yes | string | merged-source-list.fits | |
Merged source list from merge_source_list
| ||||
prefix | yes | string | 1S001 | |
Exposure identfier.
| ||||
inmask | yes | string | mos1S001-mask-im-750-1250.fits | |
Input mask file name.
| ||||
flimtot | yes | real | ||
Combined band source flux threshold (![]() | ||||
flimsoft | yes | real | ||
Soft band source flux threshold (![]() | ||||
flimhard | yes | real | ||
Hard band source flux threshold (![]() | ||||
scale | yes | real | ||
Scale factor for W90 radius.
| ||||
seper | yes | real | ||
Minimum allowed source separation in arc second.
| ||||
maxlikelim | yes | real | ||
Minimum accepted value for the maximum likelihood detetion parameter.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
caldb | yes | string | ||
Directory containing all the ESAS specific calibration files
| ||||
dirfile | yes | string | mydir | |
File containing the list of exposures, including the
directory string, for data to be merged. For instance, if the merging
processing is being done in the directory /DATA/merge and the
individual observations are located in the parallel directories
/DATA/obs1/proc and /DATA/obs2/proc, the file dirlist
could have entries such as:
/DATA/obs1/proc/mos1S001 /DATA/obs1/proc/mos2S002 /DATA/obs1/proc/pnS003 /DATA/obs2/proc/mos1S001 /DATA/obs2/proc/mos2S002 /DATA/obs2/proc/pnS003 | ||||
coord | yes | int | 1 | |
Selects which coordinate system should be used,
1: ecliptic, 2: equatorial, 3: galactic.
| ||||
crvaln1 | yes | real | ||
Central longitude of the projection.
| ||||
crvaln2 | yes | real | ||
Central latitude of the projection.
| ||||
pixelsize | yes | real | ||
Pixel size of the projection in decimal degrees.
| ||||
component | yes | int | 1 | |
Component to be cast, 1: count image, 2: exposure, 3: QPB counts, 4: SP counts..
| ||||
alpha | yes | real | 1.7 | |
Assumed spectral index for the filter correction scaling.
| ||||
elow | yes | int | 400 | |
Energy low limit (in eV) for the band.
| ||||
ehigh | yes | int | 1250 | |
Energy high limit (in eV) for the band.
| ||||
maskcontrol | yes | int | 1 | |
Mask control, 0: no masking, 1: point source masking
using the output from cheese, 2: good area masking using the masks
produced by mos-spectra, 3: mask from merged source list
output from make_mask_merge.
| ||||
xdim | yes | int | 2000 | |
X dimension of the output image
| ||||
ydim | yes | int | 2000 | |
Y dimension of the output image
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
dirfile | yes | string | mydir | |
File containing the list of ObsID directory strings for source
lists to be merged. For instance, if the merging
processing is being done in the directory /DATA/merge and the
individual observations are located in the parallel directories
/DATA/obs1/proc and /DATA/obs2/proc, the file dirlist
could have entries such as:
/DATA/obs1/proc/ /DATA/obs2/proc/ | ||||
maxlikelim | yes | real | ||
Minimum accepted value for the maximum likelihood detetion parameter.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
prefix | yes | string | S003 | |
Detector and exposure identifier,(e.g., 1S001 for MOS1 S001 exposure).
| ||||
caldb | yes | string | ||
Directory containing all the ESAS specific calibration files
| ||||
diag | yes | int | 1 | |
Controls the amount of diagnostic output (0 low, 1 medium, 2 high)
| ||||
elow | yes | int | 400 | |
Energy low limit (in eV) for the band.
| ||||
ehigh | yes | int | 1250 | |
Energy high limit (in eV) for the band.
| ||||
ccd[1-7] | yes | int | 1 | |
Selects which ccd's should be included.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
prefix | yes | string | 1S001 | |
Detector and exposure identifier (eg. "1S001") for MOS1 S001 exposure
to be processed.
| ||||
caldb | yes | string | ||
Directory containing all the ESAS specific calibration files
| ||||
region | yes | int | reg.txt | |
the selection expression for the desired region for the
generation of the model background spectrum. If no file with the input name
exists, or if the file is empty, then the default is to model the data from
the entire field of view. If a specific region is desired, the region
expression must be in detector coordinates. For example, a file containing
&&((DETX,DETY) IN circle(201,-219,3600)) would extract the central
![]() | ||||
mask | yes | int | ||
Flag to mask out point sources. 0 selects no masking
while 1 will cause mos-spectra to use the output filtered source
region file from cheese or cheese-bands.
| ||||
elow | yes | int | 400 | |
Energy low limit (in eV) for the band. If
elow and ehigh are set to 0, the image processing will
be eliminated and only spectral files will be produced.
| ||||
ehigh | yes | int | 1250 | |
Energy high limit (in eV) for the band. If
elow and ehigh are set to 0, the image processing will
be eliminated and only spectral files will be produced.
| ||||
ccd1-7 | yes | int | 1 | |
Flag to include individual CCDs. 1 to include, 0 to not.
| ||||
prefix | yes | string | S003 | |
Detector and exposure identifier,(e.g., S003 exposure).
| ||||
caldb | yes | string | ||
Directory containing all the ESAS specific calibration files
| ||||
diag | yes | int | 1 | |
Controls the amount of diagnostic output (0 low, 1 medium, 2 high)
| ||||
elow | yes | int | 400 | |
Energy low limit (in eV) for the band.
| ||||
ehigh | yes | int | 1250 | |
Energy high limit (in eV) for the band.
| ||||
quad[1-4] | yes | int | 1 | |
Selects which PN quadrants should be included.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
prefix | yes | string | 1S001 | |
Detector and exposure identifier (eg. "S001") for the PN S001 exposure
to be processed.
| ||||
caldb | yes | string | ||
Directory containing all the ESAS specific calibration files
| ||||
region | yes | int | reg.txt | |
the selection expression for the desired region for the
generation of the model background spectrum. If no file with the input name
exists, or if the file is empty, then the default is to model the data from
the entire field of view. If a specific region is desired, the region
expression must be in detector coordinates. For example, a file containing
&&((DETX,DETY) IN circle(201,-219,3600)) would extract the central
![]() | ||||
mask | yes | int | ||
Flag to mask out point sources. 0 selects no masking
while 1 will cause pn-spectra to use the output filtered source
region file from cheese-bands.
| ||||
elow | yes | int | 2000 | |
Energy low limit (in eV) for the band. If
elow and ehigh are set to 0, the image processing will
be eliminated and only spectral files will be produced.
| ||||
ehigh | yes | int | 7200 | |
Energy high limit (in eV) for the band. If
elow and ehigh are set to 0, the image processing will
be eliminated and only spectral files will be produced.
| ||||
quad1-4 | yes | int | 1 | |
Flag to include individual quadrants.
| ||||
func | yes | string | mateos | |
Name of logN-logS function.
hms (Hasinger, Miyaji, & Schmidt 2005) mushotzky (REF TBD) cappelluti (Cappelluti et al. 2008) mateos (Mateos et al. 2008) | ||||
min_src_flux | yes | real | 1.0e-14 | |
Source flux cutoff in erg/cm2/s.
| ||||
cxrb_norm | yes | real | 10.6 | |
Normalization of the cosmic X-ray background.
| ||||
index | yes | real | 1.46 | |
Photon power law index.
| ||||
prefix | yes | string | ||
Detector and exposure identifiers (eg. "1S001") for the MOS exposure
S001) to be processed.
| ||||
caldb | yes | string | ||
Directory containing all the ESAS specific calibration files
| ||||
ccd[1-7] | yes | string | 1 | |
Flag to include (1) or not (0) a CCD.
| ||||
elow | yes | int | 400 | |
The low energy for the band in eV
| ||||
ehigh | yes | int | 1250 | |
The high energy for the band in eV
| ||||
spectrumcontrol | yes | int | 1 | |
1 for a power law model, 2 for a broken power law
| ||||
pindex | no | unknown | ||
Fitted power law index, only if spectrumcontrol=1
| ||||
pnorm | no | unknown | ||
Scale factor for power law index, only if spectrumcontrol=1
| ||||
binds | no | unknown | ||
Fitted soft broken power law index, only if spectrumcontrol=2
| ||||
bbreak | no | unknown | ||
Break energy for broken power law model, only if spectrumcontrol=2
| ||||
bindh | no | unknown | ||
Fitted hard broken power law index, only if spectrumcontrol=2
| ||||
bnorm | no | unknown | ||
Normalization for broken power law, only if spectrumcontrol=2
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
caldb | yes | string | ||
Directory containing all the ESAS specific calibration files
| ||||
mode | yes | int | 1 | |
mode - 1: do a single region, 2: do multiple regions with the
required input provided in a text file (parameter spfile).
| ||||
det | yes | int | 1 | 1|2|3 |
FOR MODE=1 - Detector, 1 for MOS1, 2 for MOS2,
and3 for PN
| ||||
maskfile | yes | string | region | |
FOR MODE=1 - File name for the mask file. This is the
mosprefix-obj-im-sp-det.fits file produced for the
region by mos-spectra.
| ||||
specfile | yes | string | specfile | |
FOR MODE=1 - File name for the spectral file for the region.
| ||||
spfile | yes | string | ||
FOR MODE=2 - ASCII text file with the input for multiple regions. The
file should contain, on separate lines, the detector number (det),
mask file name (mask), and spectral file name (spec) for each region.
| ||||
mode | yes | int | 1 | |
Selection on particle (1), soft proton (2), SWCX (3) backgrounds,
(4) MASK, (5) MASKIT.
| ||||
prefix | yes | string | 1S001 | |
Detector and exposure identifiers (eg. "1S001") for the MOS exposure
S001) to be processed.
| ||||
elow | yes | int | 350 | |
The low energy for the band in eV
| ||||
ehigh | yes | int | 800 | |
The high energy for the band in eV
| ||||
detx | yes | int | ||
The DETX reference pixel location
| ||||
dety | yes | int | ||
The DETY reference pixel location
| ||||
skyx | yes | int | ||
The X location of the reference pixel
| ||||
skyy | yes | int | ||
The Y location of the reference pixel location
| ||||
maskfile | yes | string | ||
The file name for an image to provide additional masking
if desired. If left blank then there will be no additional masking.
The mask images must be the same size and projection of the other images.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
prefix | yes | string | 1S001 | |
Detector and exposure identifiers (eg. "1S001") for the MOS exposure
S001) to be processed.
| ||||
mask | yes | string | none | |
The file name for an image to provide additional masking
if desired. If left blank then there will be no additional masking.
The mask images must be the same size and projection of the other images.
| ||||
elow | yes | int | 400 | |
The low energy for the band in eV
| ||||
ehigh | yes | int | 1250 | |
The high energy for the band in eV
| ||||
mode | yes | int | 1 | |
Selection on particle (1), soft proton (2), SWCX (3) backgrounds,
(4) MASK, (5) MASKIT.
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
caldb | yes | string | 1S001 | |
Directory containing the ESAS calibration files.
| ||||
detector | yes | int | 1 | |
Detector to be processed 1-MOS1, 2-MOS2, and 3-PN.
| ||||
fullimage | yes | string | mos1S001-sp-ps.fits | |
Image from the full field of view.
| ||||
fullspec | yes | string | mos1S001-obj-ps.pi | |
Spectrum from the full field of view.
| ||||
regionimage | yes | string | mos1S001-sp-nps.fits | |
Image from the selected region.
| ||||
regionspec | yes | string | mos1S001-obj-nps.pi | |
Spectrum from the selected region.
| ||||
rnorm | yes | real | 0.05 | |
Xspec normalization of the SP component.
| ||||
prefix | yes | string | ||
Detector and exposure identifiers (eg. "1S001") for the MOS exposure
S001) to be processed.
| ||||
caldb | yes | string | ||
Directory containing all the ESAS specific calibration files
| ||||
ccd[1-7] | yes | string | 1 | |
Flag to include (1) or not (0) a CCD.
| ||||
elow | yes | int | 400 | |
The low energy for the band in eV
| ||||
ehigh | yes | int | 1300 | |
The high energy for the band in eV
| ||||
elinelist | yes | unknown | 1 2 | |
Energies of SWCX lines to be included
| ||||
gnormlist | yes | unknown | 0.1 0.03 | |
Gaussian normalizations from Xspec
| ||||
objrmf | yes | string | ||
RMF for the region
| ||||
objarf | yes | string | ||
ARF for the region
| ||||
objspec | yes | string | ||
Spectrum for the region
| ||||
clobber | no | boolean | yes | T/F |
Clobber existing files?
| ||||
Parameter | Mand | Type | Default | Constraints |