README.txt -- Description of Files and Other Data Products:

allvars.dat        Variable star photometry; same as varstd_vri.* 
		    but all in one big file.

asas_id1_data.txt  ASAS time-magnitude data for ID#1 = ASAS 190744+0007.1

asas_id1_lc.eps	   Time-magnitude plot for ID#1 = ASAS 190744+0007.1

cmd_v_vi.eps	   Color-magnitude diagram for P5 field with var* ID#s

compstar_vri.tvm   Positions & magnitudes for 16 comparison stars, the
		    XY coordinates correspond to finder_bg.fits.

finder_bg.fits	   FITS image of the Bowling Green (BG) field

finder_p5.fits	   FITS image of the PROMPT#5 (P5) field

phi_vi.*.eps	   Phased light curve plot for stars with ID# = *

ref.eps		   Photometry of a non-variable reference star to
		    demponstrate quality of time-series photometry.

spectrum.eps	   ChamPLane spectrum of NVS 11749 from Fig.1 of the paper

spectrum.dat       Data for spectrum (wavelength, counts; not flux calibrated)

time_mag_3short.eps   Time-magnitude plot for ID#417 for the 3 nights
			with high-cadence observations.

vars_vri.tvm       Positions & magnitudes for the 10 variable stars, the
		    XYbg coordinates correspond to finder_bg.fits and
		    the XYp5 coordinates correspond to finder_p5.fits.

varstd_vri.*	   Full photometry for each variable star ID# = *,
                    with the following format:

column  Contents
 1	mHJD	Heliocentri Julian Date - 2,450,000 days
 2	Vmag	Median V mag from diff'l photom from NcompV comp stars
 3	Ver1    Mean of the NcompV individual magnitude errors
		 (includes errors in comp and var aperture mags, error
		  in standard mag of comp, and error in color term) 
 4	Ver2    Standard error of the mean from NcompV indiv mag values*
 5	NcompV  Number of comparison stars used 
 6	Rmag	As Vmag, but for R
 7	Rer1	As Ver1, but for R
 8	Rer2    As Ver2, but for R*
 9	NcompR  As NcompV but for R
10	Imag	As Vmag, but for I
11	Ier1	As Ver1, but for I
12	Ier2	As Ver2, but for I*
13	NcompI	As NcompV but for I
14	SM	supermongo point style, 41=poor seeing, 90=good seeing
15	FWHM	in pixels
16	Airmass
17	Ncomp	number of comparison stars tried
18	File	original image name

*NB: we prefer to use the second error to describe the random, point
 to point photometric error, recognizing that the entire light curve
 may be shifted up/down by systematic errors in the photometric
 zero-point.


varstd_vri_t.*	   Photometry for each variable star ID#=*, where
                    multiple observations on each night were 
                    averaged, in the following format:

column  Contents
 1	mHJD	Heliocentri Julian Date - 2,450,000 days
 2	Vmag	Median V mag from diff'l photom from NcompV comp stars
 3	Verr	Standard error of the mean indiv mag values that night
 4	NcompV  Number of comparison stars used 
 5	Rmag	As Vmag, but for R
 6	Rerr	As Verr, but for R
 7	NcompR  As NcompV but for R
 8	Imag	As Vmag, but for I
 9	Ier1	As Ver1, but for I
10	NcompI	As NcompV but for I
11	SM	supermongo point style, 41=poor seeing, 90=good seeing
12	FWHM	in pixels
13	Airmass
14	Ncomp	number of comparison stars tried
15	File	original image name


For questions, please contact Andy Layden, laydena@bgsu.edu  (2013/08/13)
