This page (revision-16) was last changed on 07-Dec-2016 14:14 by JianSun

This page was created on 19-Jul-2007 12:47 by LouiseHarra

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Version Date Modified Size Author Changes ... Change note
16 07-Dec-2016 14:14 17 KB JianSun to previous
15 10-Nov-2008 10:25 17 KB JianSun to previous | to last
14 10-Nov-2008 10:21 17 KB JianSun to previous | to last
13 10-Nov-2008 10:21 17 KB JianSun to previous | to last
12 10-Nov-2008 10:21 17 KB JianSun to previous | to last
11 10-Nov-2008 06:56 17 KB David R Williams to previous | to last
10 07-Nov-2008 10:03 17 KB JianSun to previous | to last
9 05-Nov-2008 14:50 17 KB JianSun to previous | to last
8 05-Nov-2008 14:49 17 KB JianSun to previous | to last
7 05-Nov-2008 14:04 7 KB JianSun to previous | to last
6 05-Nov-2008 14:02 8 KB JianSun to previous | to last
5 05-Nov-2008 12:52 8 KB JianSun to previous | to last
4 05-Nov-2008 12:24 4 KB JianSun to previous | to last
3 05-Nov-2008 12:20 4 KB JianSun to previous | to last
2 19-Jul-2007 13:53 2 KB LouiseHarra to previous | to last
1 19-Jul-2007 12:47 2 KB LouiseHarra to last

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At line 9 changed one line
__eis_data__getwindata.pro__ : Returns EIS data from a detector window.
__eis_data~__getwindata.pro__ : Returns EIS data from a detector window.
At line 11 changed one line
__eis_data__getwinheader.pro__: Returns the FITS header for a spectral window
__eis_data~__getwinheader.pro__: Returns the FITS header for a spectral window
At line 40 added 11 lines
__eis_prep.pro__: carries out EIS calibration
__eis_raster_browser.pro__: This routine is used to browse 3D EIS data-cubes.
__eis_spike_viewer.pro__: This tool is for browsing EIS data arrays that have been cleaned of cosmic ray hits.
__fig_tsmean.pro__: plots temporal mean of spectrum
__line_centroid.pro__: Finds the centroid of an emission or absorption line by minmizing the function SUM( (wavel_i-ref) * flux_i ), for the centroid wavelength
__xmoment.pro__: XMOMENT plots mean line profile, and has interactive mouse functions to mark where the line is (start/stop pixels) and where the continuum is.