map-spectra

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map-spectra

map-spectra calculates the mapping between science plane (wavelength and slit coordinate) and CCD focal plane for a given observation set.

 

USAGE

map-spectra observset

INPUT

observset.obsdef name of an existing observation definition file

OUTPUT

observset.map is a file with the mapping information

PARAMETERS

minlambda

minimum wavelength

maxlambda

maximum wavelength

minpixl

minimum number of pixels of spectrum on a chip

use_partial

map partial slits

use_holes

map alignment holes as well as slits

 

Details:

map-spectra first finds, for each slit, spectrum segments- ranges of wavelength- that fall on each chip. Wavelengths at which the object position along the slit is too close (a few pixels) to the chip edge are not included. If <span style="font-size:11.0pt;font-family:"Courier New"; font-weight:normal">minpixl</span><span style="font-size:12.0pt;font-weight: normal"> is set to a non-zero number, shorter segments are discarded. </span><span style="font-size:12.0pt">map-spectra</span><span style="font-size:12.0pt; font-weight:normal"> does not map <i>partial</i> slits, those with an end which falls off the edge of the CCD at any wavelength, unless </span><span style="font-size:11.0pt;font-family:"Courier New";font-weight:normal">use_partials</span><span style="font-size:12.0pt;font-weight:normal"> is set to </span><span style="font-size:11.0pt;font-family:"Courier New";font-weight:normal">&#8220;y&#8221;</span><span style="font-size:12.0pt;font-family:"Courier New";font-weight:normal">. </span><span style="font-size:12.0pt;font-weight:normal">If partial slits are mapped, map-spectra finds the wavelength at which the smallest fraction of the slit is on a ccd, and uses this length for the entire spectrum. Slits that are not mapped, and partial slits that are mapped, are reported when the program exits. You must set <code><span style="font-family:"Times New Roman",serif">use_holes</span></code> to &quot;y&quot; if you intend to use the alignment stars during the extraction in </span><span style="font-size:12.0pt;font-weight:normal">extract-2dspec</span><span style="font-size:12.0pt;font-weight:normal">.</span> </h3> <h3 style="margin-left:.5in;text-indent:-.25in"><span style="font-size:12.0pt; font-family:Symbol;font-weight:normal">&middot;<span style="font:7.0pt "Times New Roman"">&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; </span></span><span style="font-size:12.0pt;font-weight:normal">partial slits may require special handling in later steps of the reduction. See the documentation of </span><span style="font-size:12.0pt">adjust-map</span><span style="font-size:12.0pt;font-weight:normal"> and the COSMOS Cookbook for details. </span></h3> <h3 style="margin-left:.5in;text-indent:-.25in"><span style="font-size:12.0pt; font-family:Symbol;font-weight:normal">&middot;<span style="font:7.0pt "Times New Roman"">&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; </span></span><span style="font-size:12.0pt">map-spectra</span><span style="font-size:12.0pt;font-weight:normal"> may not handle slits that are longer than the width of a ccd chip.</span></h3> <p class="MsoNormal">&nbsp;</p> <p><a href="../docs/Programs.html">Back to Programs</a> </p> </div>