Supplemental data for Abbas et al. 2014: "Variable Stars in Metal-Rich
Globular Clusters: IV. Long Period Variables in NGC 6496"

Filename          Contents

n6496.ps	  Paper accepted for publication in PostScript.

n6496i.fits	  I-band FITS image from PROMPT.  
n6496v.fits	  V-band FITS image from PROMPT.  
finder_p4.ps	  V-band image with variables marked.

daom_vi.std	  Mean photometry (V, I) calibrated to Stetson, 
		  with X,Y corresponding to image n6496i.fits.  
		  Full version of Table 2 from paper.

daom_vi.std_vars  Mean photometry and P4 positions of variable stars.
table5.txt	  Table 5.
cmd3.eps	  CMDs in VI from Figure 3 of the paper.

n6496v_09m.fits	  V-band FITS image from CTIO 0.9m, 1996.  
vars.ctio.tvm     Positions of variable stars on CTIO 0.9m image.
daom_VIctio.std	  Mean photometry from CTIO 0.9m 1996, matches image XY.

time_series.txt   Table 4 with last 5 columns defined below.

lc_6lpv.eps       Figure 5.
tVI_V**.dat	  Time vs magnitude data for Vnn (V01-V08=LPVs + V14, 
   which is a suspected variable not discussed in the published
   paper).  These data are in Table 4, but have a longer format here:
	col  1: f10.4   Time of observation, Julian Date - 2,450,000 days
	col  2: f8.3    I-band magnitude (long exposure, I_L)
	col  3: f6.3    Internal* uncertainty in I_L magnitude
	col  4: f6.3    External** uncertainty in I_L magnitude
	col  5: i3      Number of comparison stars used in I_L
	col  6: f8.3    I-band magnitude (short exposure, I_S)
	col  7: f6.3    Internal* uncertainty in I_S magnitude
	col  8: f6.3    External** uncertainty in I_S magnitude
	col  9: i3      Number of comparison stars used in I_S
	col 10: f8.3    V-band magnitude
	col 11: f6.3    Internal* uncertainty in V magnitude
	col 12: f6.3    External** uncertainty in V magnitude
	col 13: i3      Number of comparison stars used in V
	col 14: i3      Supermongo point style
	col 15: f5.1    Typical seeing on image (fwhm in pixels)
	col 16: f6.1    Airmass at mid-exposure
	col 17: i3      Number of comparion stars available
	col 18: a9      Image name
  * internal error is quadratic sum of DAOPHOT photometry errors (var
   & comp), standard error of comp, and color term.
  ** external error is SD/sqrt(N) of mag estimates from N comp stars.
tVI_V**.eps	  Light cuves for LPVs (V01-08).

lc_6spv.eps       Figure 7.
lc_V**.eps	  Phased light cuves for SPVs (V09-13).
tp_V*.dat	  Individual light curve data for short period
		   variables (V9-V13); format as for tVI_V**.dat
		   except col 2 contains phase.

asas_175901_44115_vdata.dat    ASAS photometry (which see for format)
asas_www.eps      ASAS light curve phased with P=740d.

coordinate_table.txt   Table 3.
cmd_JK.eps	  2MASS JK CMD of all stars within 5 armin of cluster
		  with variable stars marked.
