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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2187
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dc.contributor.authorKashyap, V-
dc.contributor.authorDrake, J. J-
dc.date.accessioned2008-04-02T10:24:06Z-
dc.date.available2008-04-02T10:24:06Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 475 - 476en
dc.identifier.urihttp://hdl.handle.net/2248/2187-
dc.description.abstractPINTofALE was developed to analyze spectroscopic data from coronal sources in the 1-1500 Å range. It is based on a modular set of IDL tools that interact with an atomic database and with observational data. The tools allow us to easily identify spectral lines, measure fluxes, and carry out more detailed modeling. The package has been extended to handle analysis of high-resolution X-ray spectra that will be obtained with the Chandra X-ray Observatory.en
dc.format.extent199804 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..475Ken
dc.subjectX-raysen
dc.subjectX-ray Spectroscopyen
dc.subjectStellar coronaeen
dc.subjectAnalysis methodsen
dc.titlePINTofALE : Package for the interactive analysis of line emissionen
dc.typeArticleen
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