N.        Date         Object       UT start  expt  airmass    slit       range     format
                                                sec

38175   25 Feb 2002       HD 26793   17:53:02   300  1.269  200 East-West  9500-4500 26 orders         
38176   25 Feb 2002       HD 26793   18:05:32   300  1.270  200 East-West  9500-4500 26 orders         
38178   25 Feb 2002       HD 26793   18:17:03   300  1.287  200 East-West  9500-4500 26 orders
38181   25 Feb 2002       V838 Mon   19:24:56   600  1.589  200 East-West  9500-4500 26 orders         
38182   25 Feb 2002       V838 Mon   19:38:20  1200  1.556  200 East-West  9500-4500 26 orders         
38184   25 Feb 2002       V838 Mon   20:05:11  1200  1.555  200 East-West  9500-4500 26 orders         

38379   26 Mar 2002       V838 Mon   18:40:56  1200  1.589  200 East-West  9500-4600 25 orders       
38381   26 Mar 2002       V838 Mon   19:27:51  1200  1.701  200 East-West  9500-4600 25 orders       

        HD26793 is an early type, fast rotating star useful to 
        locate telluric absorptions and to check for glinches
        in the flat-field

 The spectra have been secured with the Echelle+CCD spectrograph on
 the 1.82 m telescope operated by Osservatorio Astronomico di Padova atop Mt.
 Ekar (Asiago) and make available to us by U.Munari (2003, private
 communication). A 2 arcsec slit was adopted with fixed E-W orientation,
 producing a PSF with a FWHM of 1.75 pixels, corresponding to a resolving
 power close to 20000. The detector has been a UV coated Thompson CCD
 1024x1024 pixel, 19 micron square size, covering in one exposure from 4500
 to 9480~\AA\ (from Echelle order \#49 to \#24). The short wavelength limit
 is set by a 2~mm OG~455 long-pass filter, inserted in the optical train to
 cut the second order from the cross-disperser. The wavelength range is
 covered without gaps between adjacent Echelle orders up to 7300~\AA. The
 spectra have been extracted and calibrated in a standard fashion with IRAF
 running under Linux operating system. The spectra are sky-subtracted and
 flat-fielded.  The wavelength solution has been derived simultaneously for
 all 26 recorded Echelle orders, with an average r.m.s of 0.18~km~sec$^{-1}$.
 The 8480-8750~\AA\ wavelength range of these Asiago spectra has been
 described in Munari et al. (2002a, b)

 Munari, U. et al. 2002a, A\&A 389, L51
 Munari, U. et al. 2002b, in "Classical Nova Explosions", M.Hernanz and
         J.Jos\'{e} eds., AIP Conf. Ser. 637, 52