______________________________________________________________________________ DG DISPGAL is a module which plots galaxian photometric and structural parameters and fits various curves to them. It requires data to be in a file of type 3. ______________________________________________________________________________ Enter an option: 25-NOV-1991 16:49:00.16 OPTION=DG DISPGAL, Version 2 Enter a command: R = Plots radius-parameter against magnitude (default) S = Plots surface brightness against magnitude T = Plots surface brightness against radius-parameter M = Plots the mean error against magnitude D = Displays the differential luminosity function I = Displays the integrated luminosity function I2 = Displays two integrated luminosity functions C2 = Plots the integrated color (first file minus second) against magnitude of the first file C2C = Plots the magnitude of one file against that of another G2 = Plots color gradient and color delta against magnitude or against each other as derived from two files S2 = Plots surface brightness color against magnitude S2S = Plots surface brightness of one file against that of another A2 = Plots the average radius-parameter against magnitude R2 = Plots the ratio of radius-parameter against magnitude R2R = Plots the radius-parameter of one file againstthat of another M2 = Plots the ratio of mean error against magnitude COMMAND=G2 Do you want to plot a curve through the data? (default = Y) CURVE_FIT= T ....Our intention is to plot a straight line by least squares Enter the lower limit of acceptance for the radius-parameter: (default = 0.0) LOWER_LIMIT=.001 ....This file contains some faint magnitudes without radius parameters, so we must put in this limit Enter the lower limit of acceptance for the magnitude: (default = -100.00) LOWER_LIMIT_MAGNITUDE= -100.000 Enter the upper limit of acceptance for the magnitude: (default = 100.00) UPPER_LIMIT_MAGNITUDE=18 ....The very faintest data is too noisy Open the first data file to be plotted Enter the file name: (default = last entry) FILE_21=G022152 ....The blue parameters in a file of type 3 Open the second data file to be plotted Enter the file name: (default = last entry) FILE_22=G022151 ....The red parameters Enter a choice: GH = Dimensionless color gradient (linear in r) for the Hubble formula against magnitude. The files must contain Hubble a's DH = Color delta for the Hubble formula against magnitude (default) The files must contain Hubble a's. DV = Color delta for the de Vaucouleurs formula against magnitude The files must contain de Vaucouleurs r's. HV = Color delta for the Hubble and de Vaucouleurs formulas against each other CHOICE=DH Enter the radius as a multiple of the radius parameter: (default =1) RADIUS= 1.00000 ....The color delta is calculated as the difference in color between center and, in this case, 1 radius parameter away from the center. Do you wish to plot the error bars? (default = Y) ERROR_BARS= T ID MH COLOR DELTA 17 -0.6674 +- 0.1095 59 0.2666 +- 0.0764 70 -0.0703 +- 0.0340 72 -0.0216 +- 0.0584 85 -0.0663 +- 0.0624 104 -0.0459 +- 0.0945 114 -0.0050 +- 0.0895 123 -0.1680 +- 0.0751 126 0.0096 +- 0.0590 129 -0.3938 +- 0.0489 144 0.3511 +- 0.0805 147 -1.1310 +- 0.1205 161 -0.1816 +- 0.0952 ....Here are the color deltas and their errors Enter the degree of the polynomial fit: (default = 0) DEGREE=1 Do you want to force the curve through the brightest point? (default = N) FORCE= F Do you want to fix the constant? (default = Y) FIX_CONSTANT=N Do you want to fix the slope? (default = Y) FIX=N ORDER COEFFICIENT MEAN ERROR 0 0.13363 2.8492 1 -0.17197E-01 0.16486 ....The least squares parameters Enter the plot devices: G = Graphics terminal (VT100/Retrographics and Visual 550, default) G1 = Graphics terminal (GraphOn) G2 = Graphics terminal (Codonics) G3 = Graphics terminal (Micro-term) F = File T = Tektronix 4662 flat bed plotter (1200 baud) DEVICES= G ....The plot looks OK Do you want to plot the residuals about the mean fit? (default = Y) RESIDUALS= T Enter the bin size in magnitudes: (default = 0.10) INTERVAL= 0.100000 Enter the plot devices: G = Graphics terminal (VT100/Retrographics and Visual 550, default) G1 = Graphics terminal (GraphOn) G2 = Graphics terminal (Codonics) G3 = Graphics terminal (Micro-term) F = File T = Tektronix 4662 flat bed plotter (1200 baud) DEVICES= G ....There is a slight assymmetry ....We could go back and change any input parameter with the .DG(KEYWORK=...) option. We could also interact with the plot to produce a camera ready copy. ....Here is another example of option DG. Enter an option: 25-NOV-1991 16:42:57.19 OPTION=DG DISPGAL, Version 2 Enter a command: R = Plots radius-parameter against magnitude (default) S = Plots surface brightness against magnitude T = Plots surface brightness against radius-parameter M = Plots the mean error against magnitude D = Displays the differential luminosity function I = Displays the integrated luminosity function I2 = Displays two integrated luminosity functions C2 = Plots the integrated color (first file minus second) against magnitude of the first file C2C = Plots the magnitude of one file against that of another G2 = Plots color gradient and color delta against magnitude or against each other as derived from two files S2 = Plots surface brightness color against magnitude S2S = Plots surface brightness of one file against that of another A2 = Plots the average radius-parameter against magnitude R2 = Plots the ratio of radius-parameter against magnitude R2R = Plots the radius-parameter of one file againstthat of another M2 = Plots the ratio of mean error against magnitude COMMAND= R Do you want to distinguish those galaxies within a certain distance from a defined center? (default = N) DISTINGUISH= F Enter the lower limit of acceptance for the radius-parameter: (default = 0.0) LOWER_LIMIT=.001 ....Some galaxies may not have radius parameters Enter the lower limit of acceptance for the magnitude: (default = -100.00) LOWER_LIMIT_MAGNITUDE= -100.000 Enter the upper limit of acceptance for the magnitude: (default = 100.00) UPPER_LIMIT_MAGNITUDE= 100.000 ....We'll plot them all Open the data file to be plotted Enter the file name: (default = last entry) FILE_21=G022152 The centroid of the X values is: 18.9605 The centroid of the Y values is: -0.8665 ....This gives us a feel for the starting values for the nonlinear least squares fit about to be done. The plot contains 119 points Do you want to plot a single curve through the data? (default = N) CURVE_FIT= F Enter a choice: A = Solves for m' and log(r') and plots the result (default) B = Solves for m',log(r'), and the slopes, and plots the result C = No fitting FIT_CHOICE=B Enter the weighting scheme: E = Equal weights (default) M = According to mean error WEIGHTING_SCHEME= E Enter the estimates for m' and log(r'): ESTIMATES=18.9 0.9 ....From above m' = 17.8686 +- 0.5399 ....This is the magnitude of the intersection of two straight lines. Other parameters of the fit and their errors will appear on the screen. Mean error for an observation of average weight = 0.1816 Enter the plot devices: G = Graphics terminal (VT100/Retrographics and Visual 550, default) G1 = Graphics terminal (GraphOn) G2 = Graphics terminal (Codonics) G3 = Graphics terminal (Micro-term) F = File T = Tektronix 4662 flat bed plotter (1200 baud) DEVICES= G ______________________________________________________________________________