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Environment with several tools for Pacs molecular spectroscopy managing.
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Inherited from Inherited from |
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Inherited from |
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Initializing an instance of Pacs().
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Read the data from the line fit procedure done with Pierres Hipe script. Assumes structure and syntax as given in the example file /home/robinl/Data/PACS/v1362aql/lineFit/lineFitResults The line fit results are saved in self.linefit as a np.recarray. The columns include (with unit indicated): groupid band wave_in (micron), wave_fit (micron), line_flux (W/m2), line_flux_err (W/m2), line_flux_rel (%), continuum (W/m2 m), line_peak (W/m2 m), fwhm_fit (micron), fwhm_pacs (micron), fwhm_rel
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Set parameters taken from the PACS database into empty parameter sets. Typically used in conjunction with making Star() templates through Star.makeStars().
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Read data from given filenames and remember them. If no filenames given, an auto search is performed. The data are saved as wavelength and flux lists in the object.
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Prepare Sphinx PACS models by checking if the Star() instance already has a PACS id associated with it, and if not calling convolveSphinx.
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Read the sphinx convolution and return if it has already been done. Returns None if the convolution is not available.
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Check if sphinx output has already been convolved (pacs db) and do so if not.
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Get the Pacs resolution from cc aux file for all orders.
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Read and remember the PACS resolution, based on the wavelength grid of the data. Returns a list of deltas for every filename, within a list. |
Check if for this star the convolution has already been done.
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