The Spectral Correlation Function (SCF) is a diagnostic tool which scans spectral-line maps quantifying the correlation
amoungst spectra at different positions and spatial lags within a map.
SCF Code
(Most up to date SCF code and instructions.)
This page contains the following resources.
Publications and Papers
-
Padoan, Goodman, & Juvela 2003, The Spectral Correlation Function of Molecular Clouds: A Statistical Test for Theoretical Models
-
Ballesteros-Paredes, Vazquez-Semadeni, & Goodman 2002, Velocity Structure of the Interstellar Medium as Seen by the Spectral Correlation Function
-
Padoan, Kim, Goodman, & Staveley-Smith 2001, A New Method to Measure and Map the Gas Scale Height of Disk Galaxies
-
Padoan, Rosolowsky, & Goodman 2001, The Effects of Noise and Sampling on the Spectral Correlation Function
-
Rosolowsky, Goodman, Wilner, & Williams 1999, The Spectral Correlation Function: A New Tool for Analyzing Spectral Line Maps Data Page for this Paper
Old Source Codes
The SCF algorithm is written for IDL 4.0.1 and is compatible
with IDL 5.0.x, (though not optimized).
There are three basic distributions of the SCF code:
- The original SCF distribtution.
- A minimal SCF distribution.
- The GUI SCF distribution.
If you have questions or comments about the SCF project
or would like to submit data for analysis by the SCF algorithm, please contact
agoodman@cfa.harvard.edu.
Alyssa Goodman's Home
Page