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Commands in SPECPR
The following lists the commands used in SPECPR. Many commands are of a general nature and are used throughout the programs. Listed in brackets are the sections of the users manual where the commands are found. Listed in the curly brackets {} are additional options to the command letters. HTML-IMAGE.nr 3c 0
- A -
a:
Change default wavelength record assignment (general command used in Math Operations [section 8], CRT Plot Routines [section 9], and File Display, Transfer and Overlay [section 10])
a: |
Average option in addition mode [8.3]
a: |
Wavelength plot mode in CRT plot routines [9.2]
a: |
Autoscale (on CRT plot) [9.3] [10.1]
a: |
Remove all glitches and any other entered [9.6]
a: |
Assign a different wavelength record in the wavelength assignment routine
a: |
"Automatic" line printer lists of file [11.1]
a: |
Wavelength record used in plot [13.6]
a{tl}:
|
GFIT, Estimate Parameters routine to enter output file title where tl is the title, entered on same line. [14.2.1]
a{n}:
|
GFIT, Estimate Gaussians routine to change all the parameters of a gaussian, where n is the gaussian number. [14.2.2]
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- B -
b:
Change initialization parameters or return to wavelength assignment routines [7.6]
b: Turns on band normalization [8.2] [8.8] bn: Turns off band normalization [8.2] [8.8] b: Begin addition analysis [8.3] b: |
Remove all glitches in the channels identified except those specified by the user [9.6]
b: Autoscale with line printer plot [10.1] b: |
Line printer option for all header information except manual history and data [11.1]
b: Begin Building plot [13.6]
b: Begin transpose [8.6.8]
b: Begin Analysis [8.6.16] (F16)
b{xy}:
|
GFIT, Estimate Parameters routine to assign the input specpr file where x is the specpr file id and y is the record number. [14.2.1]
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- C - c:
Change channel number (wavelength assignments) [6.8]
c: |
Constant identifier in Math Operations [8.2]
c: |
Continue (after entering numbers to be deleted) [8.3]
c: Change scale (on CRT plot) [9.3] c: |
"CRT plot routine" option in file transfer mode [10.1.2]
cit: |
CRT plot of only header information and transfer [10.1.2]
c: |
Continue listing of file [11.1]
c: |
Line Printer option for all header information but not data [11.1]
c: |
Command to perform extinction calculations [12.3]
c: |
End of extinction calculations [12.3]
c: |
Connect data points in plot [13.6]
c: Continue [13.6] cp: Change protection [7.6] C: Connect points, ignore non-ordered wavelengths [13.6] c: |
Deletion ended, continue: a general command to signify end of deleted points (all routines).
co: GFIT, Plotting routine to plot the continuum [14.7]
c{n}:
|
GFIT, Estimate Parameters routine to specifying the number of continuums, where n is the number of continuums. [14.2.1]
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- D -
d:
D-file, workfile [2.2] This is a general command to access "DFILE".
d: |
Edit wavelength records (wavelength assignments) [6.9]
d{fn}:
|
Change file assignment of the d-file, where fn is the filenname [5.1]
d: |
Delete Zero’s option in addition routine [8.3]
d: |
Delete channels in addition routine [8.3], and in Gould Plot routines [13.4, 13.6]
d: |
Line printer option for all header information and data [11.1]
d: List (Display) starpack by title [12.2] d: Delete specified runs or channels [12.5] d: |
Delete specified points in smoothing function, F7 [8.6.7]
d{n}:
|
Delete step n [8.6.16] F16 Where n is an integer)
d{n}:
|
GFIT, Estimate Parameters routine for specifying the number of gaussians to be fitted, where n is the number of gaussians. [14.2.1]
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- E - e:
Exit to next routine: a general "soft exit" command
ex: |
Exit Program [7.4] (from Program Operations Control only)
e: |
Includes error bars: a general command
es: GFIT, Transfer estimate to scratch [14.4] eg: GFIT, Goto estimate gaussian routine [14.2.2] eg: GFIT, Plotting routine for erasing graphics [14.7] ep: GFIT, Goto estimate parameter routine [14.2.1] HTML-IMAGE-END |
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- F -
f: Print summary of the current restart file [7.12]
f1: Lists Index of special functions [8.6.1]
f2:
Special function, shifts data left or right an integer or fraction number of channels [8.6.2]
f3: |
Special function, sequential processor [8.6.3]
f5: Special function, continuum removal [8.6.5] f6: |
Special function, black body computation [8.6.6]
f7: Special function, smoothing [8.6.7] f8: |
Special function, channel-file transpose [8.6.8]
f9: Special function, Band Removal [8.6.9] f10: |
Special function, arranges data into increasing wavelength order [8.6.10]
f11: Special function, thermal removal [8.6.11] f12: |
Special function, cubic spline interpolation [8.6.12]
f13: Special function, merge [8.6.13] f14: Special function, Edit data [8.6.14] f15: |
Special function, Gaussian Fit Formatter [8.6.15]
f16: |
Special function, SPECPR line segment generator [8.6.16]
f17: |
Special function, High to low resolution connvolution [8.6.17]
f18: |
Special function, Block averages and statistics [8.6.18]
f19: |
Special function, Polynomial fit (10 term) [8.6.19]
f20: |
Special function, read/write data from a Unix text file in f or e format [8.6.20]
f21: |
Special function, Calculates the n-th term polynomial [8.6.21]
f22: |
Special function, reads data from the digitizing tablet, and scales it to given limits. [8.6.22]
f23: |
Special function, Mathematical expression parser. [8.6.23]
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- G -
g2: Set, White on Black graphics mode [4.6]
g3:
Compliment, White on Black graphics mode [4.6]
g11: Set, Black on White graphics mode [4.6] g13: |
Compliment, Black on White graphics mode [4.6]
g99: Not a graphics terminal [4.6]
g{n}:
|
n < 10, Jam mode, White on Black [4.6];
n > 10, Jam mode, Black on White [4.6]
g: Glitch removal routine call [9.6] g: |
Next spectrum is to be plotted on a new graph [13.6]
g: Execute GFIT prograam [7.11] g: |
Plot goodness of fit in extinction routines [12.4]
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- H -
h:
Channel plot mode in CRT plot routines [9.2] and used as a general command to indicate Channel space
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- I -
i:
Puts Program Operations Control, Math Operations, or File Display, transfer and Overlay information of the screen [7.2] [8.1]
in: |
Clears Program Operations Control information from the screen [7.2] [8.1]
i: Review and change of other information [9.5] i: Plot intercepts [12.4] in extinction routine HTML-IMAGE-END.bp HTML-IMAGE.nr 3c 0 - K - HTML-IMAGE-END.bp HTML-IMAGE.nr 3c 0 |
- L -
l:
Print the summary of the wavelength file from wavelength file assignments [6.10]
l#: |
Change line type in transfer and crt plot routines where # is the line type number, 0 = crosses only, 1 = connect crosses, 2 = connect points only, 3 = point plot [9.7]
lv: |
List v-file when in program operations control [7.3]
lw: |
List W-file when in program operations control [7.3]
ld: |
List D-file when in program operations control [7.3]
lu: |
List U-file when in program operations control [7.3]
ly: |
List Y-file when in program operations control [7.3]
l: |
"Last title" option in title routine [8.8]
l: |
Line size for axes in plot [13.6]
l: |
Set limits to data range [8.6.7] (in function F7)
l{n}:
|
List (from step n) [8.6.12] (in function F12)
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- M -
m:
Calls for math operations from Program Operations control [7.10] or File Display, Transfer and Overlay [10]
m: Command to move band limits [8.9] m: Allows changing of manual history [9.5] m: Call for manual history access [12.7] m: More copies option in plot mode [13.6] HTML-IMAGE-END.bp HTML-IMAGE.nr 3c 0 |
- N -
n: End of wavelengths [6.7]
n:
Subtraction with NO air mass calculation [8.2]
n: |
Energy space plot mode in CRT routines [9.2] and Gould Plot Routines [13.2]. Note n is second letter in energy
n: |
Command to turn line printer action off [11.1] in file list.
n: |
Delete points that lie out-of-bounds of plot [13.6]
n: Specify block size [8.6.18] (function F18) HTML-IMAGE-END.bp HTML-IMAGE.nr 3c 0 |
- O -
o:
Remove only those channels specified by user in glitch removal routine [9.6]
o: |
Calls for overlap mode in display and transfer routine [10.2]
o: |
Call for observatory location [4.3]
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- P -
p:
Generate and store nominal wavelengths of the PDS photometer (used in wavelenth assignments) [6.4]
p: Print wavelengths [6.9] p: |
Calls Gould plot routines from Program Operations Control [7.9]
p: |
Calls for Production Processing [8.2] [8.8]
p: |
"Present title" option in title routine [8.8]
pn: |
Turns Producton Processing off [8.8]
pd: |
Line printer prints header information and data [9.4]
p: Line priter plots data [9.4] p: Line priter list of file [11.1] p: |
CRT plot routine call command [12.4] in extinction routines
p: Call for Gould plot routines [13.1] p: Point size in plot mode [13.6] p: Make line printer plot of CRT plot [12.4] HTML-IMAGE-END.bp HTML-IMAGE.nr 3c 0 |
- R -
r{fn}:
Restart, where fn is the name of the restart file [4.1]
r: |
Read data from a file and put it in the wavelength file (used in wavelength assignments) [6.5]
r: |
Return to device and file assignments from Program Operations Control [7.7]
r: |
Change RA and declination in subtraction calculation [8.2]
r: |
Reinstates deleted channels [8.9] in band normalization routine
r: |
Returns to first page of information in Header Information change routines [9.5]
r: "Return" to last step [13.6]
r: Reverse energy space plot option [13.2]
r{n}:
|
Return to step n [8.6.16] function F16 (n is an integer)
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- S -
s:
Access a starpack file [2.2] in math operations [8] or File Display, Transfer and Overlay routines [10]
s: Create or list a starpack file [7.8] s: Sum option in addition mode [8.3] s: Call for extinction routines [12.1] s: |
Command to write a starpack to starpack file [12.6]
s: Change of symbol in plot print [13.6] s: Plot slopes [12.4] in extinction routines HTML-IMAGE-END.bp HTML-IMAGE.nr 3c 0 |
- T -
t:
"to" when transfering data from one file to another [10.1.1] [7.5]
t: |
Observatory location (latitude) if other than most often used observatories [4.3]
t: |
Write data from a wavelength file onto tape or disk (wavelength assignment) [6.6]
t: |
Change siderial time in subtraction routine [8.2]
t{#}:
|
title store or recall command [8.8] (#=number 1 to 25)
tl: Title list [8.8] t: |
Go to file transfer routine [11.1] from Program operations Control [7] or Math Operations [8]
t: |
Command for fitting routine [12.5] (extinction Routines)
t: |
All channels from this channel "to" that channel in delete points routines (general command in delete points routines).
t: Include text on graph [13.6] HTML-IMAGE-END.bp HTML-IMAGE.nr 3c 0 |
- U -
u: access to the "Ufile" [2.2]
u{fn}:
Change file assignment of U-file, where fn is the filename, from the file assignment routine [5.1]
u{fn}:
|
Create new restart file, where fn is the name of the restart file [4.1]
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- V -
v: Access to the "Vfile" [2.2]
v{fn}:
Change file assignment of V-file, where fn is the filename, from the file assignment routine [5.1]
v: |
Assign VIS CVF wavelengths (120 channels) in wavelength assign. routine [6.3]
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- W -
w: Access to the "Wfile" [2.2]
w:
Generate standard wavelengths of "wedge" CVF spectrometer with small calibration shift (used in wavelength assignments) [6.2]
w{fn}:
|
Change file assignment of W-file, where fn is the filename, from the file assignment routine [5.1]
w{n}:
|
GFIT, Estimate Parameters routine assign wavelength record(file) where n is the wavelength record number [14.2.1]
w: Change Horizontal wavelength scale [9.3]
w: "Wavelength" space limits [13.2]
w{n}:
|
GFIT, Estimate Gaussians routine to change the center value of a gaussian, where n is the gaussian number. [14.2.1]
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- X -
x:
Exit ("hard") from present routine. If other commands are pending, terminate all commands and return to main routine - general command.
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- Y -
y: Access to "Yfile" [2.2]
y{fn}:
Change file assignment of Y-file, where fn is the filename, from the file assignment routine [5.1]
y: |
Create your own wavelengths (wavelength assignments) [6.7]
y: User defines horizontal axis on plot [13.2] HTML-IMAGE-END.bp |