- Timestamp:
- 02/18/05 17:14:15 (20 years ago)
- File:
-
- 1 edited
Legend:
- Unmodified
- Added
- Removed
-
trunk/python/asapmath.py
r479 r481 166 166 If you specify neither, then a polynomial correction will be made 167 167 with built in coefficients known for certain telescopes (an error will 168 occur if the instrument is not known). The data a re *multiplied*168 occur if the instrument is not known). The data and Tsys are *divided* 169 169 by the scaling factors. 170 170 Parameters: … … 242 242 def opacity(scan, tau, insitu=None, allaxes=None): 243 243 """ 244 Return a scan after applying an opacity correction. 244 Return a scan after applying an opacity correction. The data 245 and Tsys are multiplied by the correction factor. 245 246 Parameters: 246 247 scan: a scantable
Note:
See TracChangeset
for help on using the changeset viewer.