dc.contributor.author |
Anandarao, B. G |
|
dc.contributor.author |
Rao, S. R |
|
dc.date.accessioned |
2006-04-10T05:40:23Z |
|
dc.date.available |
2006-04-10T05:40:23Z |
|
dc.date.issued |
1986-03 |
|
dc.identifier.citation |
BASI, Vol. 14, No. 1, pp. 25-33 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/903 |
|
dc.description.abstract |
In astronomical observations we often encounter spectra which are a result of superposition of individual contributions from phenomena of similar kind. We describe here a method together with its algorithm by which one can decompose a given set of data into a number of nonlinear functions and apply the method to a couple of astronomical data-sets. We discuss the modifications to be made in the algorithm, appropriate to the particular problem, in order to arrive at a solution. This method can be used in high-resolution spactroscopic and photometric data on astronomical objects to extract valauble information which otherwise is not apparent |
en |
dc.format.extent |
646741 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of Indian |
en |
dc.subject |
Data reduction |
en |
dc.title |
Decomposition of data into a sum of nonlinear functions Application to astronomical observations |
en |
dc.type |
Article |
en |