SED |
SED is the Spectral Energy Distribution program I decided to write after my advisor and I spent a whole afternoon trying to figure out an SED. We ended up both making errors in our hand and calculator calculations. This will hopefully eliminate that. The program is documented and menu driven so you can start from scratch and make an SED. The compliment program in SuperMongo is good for ploting the SED. It takes the output of the file from the Fortran program. Theoretically you can call SM functions from F77, but we didn't have the resources to put the proper libraries in the right directories... lazy, sorry! But you can do it if you are ambitious! |
SED1.f SED.macro |
SLIT |
This is a SM macro that makes a plot of the POS ANG, or Position Angle of a slit into a box that an image can be put in with. The other one is a prototype to create a descent grayscale in SM, it hasn't been very pretty, the tones were not coming out right, so I just did the overlay of the slit onto the image with THE GIMP. |
slit_sm.macro slit_grey.macro |
GVEL |
This program is used to quickly calculate the velocities of the gaussians I fit to the spectra of Sa 2-237, it is very selective now, you must go into it and change the parameters to use it for anything else, but it could easily be expanded to automatically read the file and dicipher the size, lines, etc, but I didn't have time for that. I incorporated a heliocentric systemic velocity parameter when I learned that the value we would get differed from the literature. Anyway, that's this one. | velocities.f |