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eso-midas-doc-13SEPpl1.2-3.mga5.i586.rpm

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<H2><A NAME="SECTION002436000000000000000">&#160;</A>
<A NAME="irspec">&#160;</A>
<BR>
irspec
</H2>
 <BLOCKQUOTE>
<TT><TT>BADPIX/IRSPEC <I>in out [l=load_opt.] [dir=clean_opt.] [debug=debug_opt.]
<BR> </I>
  </TT></TT>Clean image of fixed pattern of bad pixels <BR>
<TT>CALIBRATE/IRSPEC <I>ima
<BR> </I>
  </TT>Apply on-line (mechanical) wavelength calibration.
<BR>
<TT>CALIBRATE/IRSPEC <I>ima_ref mode=define
<BR> </I>
  </TT>Define and store in ima_ref precise calibration from sky/lamp lines
<BR>
<TT>CALIBRATE/IRSPEC <I>ima ref=ima_ref
<BR> </I>
  </TT>Apply precise wavelength calibration to frame ima from parameters
<BR>
stored in ima_ref
<BR>
<TT>DEFINE/IRSPEC <I>image table [mode] [threshold] [number] [load_option]
<BR> </I>
  </TT>Define fixed pattern of bad pixels and store it into a table.
<BR>
<TT>FLAT/IRSPEC <I>in_flat in_dark out [l=load_opt.] [t=threshold] <BR> </I>
<I>[v=vignetted_value]
<BR> </I>
  </TT>Create a normalized flat from an input flat frame.
<BR>
<TT>FLUX/IRSPEC <I>in_ima response_ima out_ima [smooth=s1,s2] [shift=sh]
<BR> </I>
<I>[norm=normalize_option] [rect=rectify_option]
<BR> </I>
  </TT>Flux calibrate a spectrum (either 2D <I>or 1D) using a response frame
<BR> </I>
  created using RESPONSE/IRSPEC
<BR>
<TT>MERGE/IRSPEC <I>prefix_ima i1,i2[,i3] out_table [excl=#pixels_excluded] <BR> </I>
<I>[corr=correct_option] [ref=#reference_image] [plot=plot_option] <BR> </I>
<I>[format=i_format]
<BR> </I>
  </TT>Merge 1D <I>spectra into a table forcing connection of overlapping regions
<BR> </I>
<TT>RECTIFY/IRSPEC <I>in out [l=load_opt.] [tilt=tilt_value] [ref=reference_row]
<BR> </I>
  </TT>Rectify tilted spectral lines.
<BR>
<TT>RESPONSE/IRSPEC <I>in_ima flux_table out_response_ima [yrows=y1,y2,y3,y4]
<BR> </I>
<I>[obs=observation_mode] [norm=normalize_option]
<BR> </I>
<I>[rect=rectify_option]
<BR> </I>
  </TT>Create a response frame from a standard star 2D <I>spectrum and
<BR> </I>
  a flux table.
<BR>
<TT>SKYSUB/IRSPEC <I>ima_obj ima_sky out factor[,shift[,deltax,deltay]]
<BR> </I>
<I>[sky=sky_table] [force=force_sky_to_zero]
<BR> </I>
<I>[cuts=cuts_values] [debug=debug_option]
<BR> </I>
  </TT>Perform obj-sky correcting for variation and shift of sky lines.
<BR>
<TT>STANDARD/IRSPEC <I>in_ascii_file out_table interp_method <BR> </I>
<I>[degree=degree] [step=wavelength_step] [limits=wl1,wl2]
<BR> </I>
<I>[units=wavelength_units] [plot=plot_option]
<BR> </I>
  </TT>Create standard star flux table from a "flux ascii file".
<BR>
<TT>SUBTRACT/IRSPEC <I>in_ima out_ima degree [exclude=area_to_exclude]
<BR> </I>
<I>[cont=continuum_image] [load=load_option]
<BR> </I>
  </TT>Fit and subtract, row by row, polynomial to a given image.
<BR>
<TT>TUTORIAL/CALIBR <BR>
  </TT>demonstration of wavelength calibration commands in IRSPEC
<BR>
<TT>TUTORIAL/IRSPEC <BR>
  </TT>General tutorial for the package IRSPEC
<BR>
<TT>TUTORIAL/SKYSUB <BR>
  </TT>Tutorial for sy substraction with IRSPEC <I>package
<BR> </I></BLOCKQUOTE><HR>
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<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-15</I>
</ADDRESS>
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