common/
ifsf_disptemp.pro
top ifsf_disptemp
IFSFIT
result = ifsf_disptemp(template, lambda, sigma [, loglam=byte])
Convolve stellar templates with a Gaussian in wavelength space. To work properly,
Return value
Convolved templates.
Parameters
- template in required type=dblarr(N,M)
Stellar continuum templates for continuum fitting, with N pixels and M templates. The template must have constant dispersion in wavelength space (default) or velocity space (if LOGLAM set).
- lambda in required type=dblarr(N)
Wavelengths
- sigma in required type=double
Sigma, in velocity velocity, of Gaussian to use in convolution.
Keywords
- loglam in optional type=byte default=0
Set to do convolution in velocity, or log(lambda), space.
Author information
- Author:
David S. N. Rupke:
Rhodes College Department of Physics 2000 N. Parkway Memphis, TN 38104 drupke@gmail.com
- Copyright:
Copyright (C) 2013 David S. N. Rupke
This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License or any later version.
This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details.
You should have received a copy of the GNU General Public License along with this program. If not, see http://www.gnu.org/licenses/.
- History:
ChangeHistory:
2009nov24 DSNR added log(lam) treatment 2013oct10, DSNR, added documentation 2013nov13, DSNR, renamed, added license and copyright
File attributes
Modification date: | Wed Nov 13 14:25:05 2013 |
Lines: | 95 |
Docformat: | rst rst |