dc.contributor.author |
Sibgatullin M. |
|
dc.contributor.author |
Kharintsev S. |
|
dc.contributor.author |
Salakhov M. |
|
dc.date.accessioned |
2018-09-17T20:59:45Z |
|
dc.date.available |
2018-09-17T20:59:45Z |
|
dc.date.issued |
2004 |
|
dc.identifier.issn |
0971-9237 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/134366 |
|
dc.description.abstract |
A comparative analysis of methods for eliminating background noise is attempted. An emphasis on the Savitzky-Golay method, Kaiser filtration and wavelet-based denoising is made; and argued that the behaviour of a singal at different scales (frequencies) plays a crucial role when the spectra are processed with the latter. |
|
dc.relation.ispartofseries |
Asian Journal of Spectroscopy |
|
dc.title |
Smoothening and denoising optical spectra of stars |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
3-4 |
|
dc.relation.ispartofseries-volume |
8 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
91 |
|
dc.source.id |
SCOPUS09719237-2004-8-34-SID27144556466 |
|