| UNDER CONSTRUCTION ... HARD HATS MANDATORY |
| Models |
Behavior of some spectral models. |
| get_fwhm.bash |
Uses source extractor and astropy to get median FWHM of an image. |
| get_mjd.py |
Uses astropy to read DATE-OBS header, and convert to MJD. |
| fluxmag.c |
Given zero point flux and magnitude (or flux), returns
flux (or magnitude). |
| redden.c |
Calculates the extinction based on Cardelli, Clayton
and Mathis 1989, ApJ, 345, 245. Given R_v, A_v and
lambda (microns), returns A_lambda. |
| deredden.csh |
Given (1) A_v (2) Bandpass (3) Magnitude, and
(4) Mag_error, find unabsorbed flux-density (Jy)
and errors using the extinction laws of
Cardelli et al. 1989 (Basically uses my redden and
fluxmag codes to get the numbers). |
| Dice |
Throwing many, many dice ... |
| expose.c |
Control a Canon EOS 300D using the parallel port. |
| rmrec |
Removes most recently created N files in the current working directory |
| jd.c |
Converts from MJD to calendar date and vice-versa using USNO routines. |
| chernoff.c |
Create Chernoff faces from N-dimensionl data
(N less than 6 for this version). An example is
here, which also requires
imagemagick's convert
tool, gnuplot and
this gnuplot script. |