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<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> <!--Navigation Panel--> <A NAME="tex2html2553" HREF="node157.html"> <IMG WIDTH="37" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="next" 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