Name:    StackResults_g-r_Mr.fits
Columns: 41
Rows:    90

This table contains the binned data plotted in Bourne et al. (2012, MNRAS, 421, 3027).
GAMA galaxies are selected as described in the paper, binned by g-r colour, M_r 
and redshift, and the stacked Herschel-ATLAS data and derived properties are calculated.
Each row of the table is one bin, defined by the limits shown below and detailed in the paper.
All errors are 1-sigma.

Bins are indexed in z, M_r, and g-r colour by the columns ZIND, MIND, CIND:
Redshift bins: (0) 0.01-0.12; (1) 0.12-0.17; (2) 0.17-0.22; (3) 0.22-0.28; (4) 0.28-0.35
M_r bins: redshift-dependent limits given in the column MLIMITS.
Colour bins: (0) blue cloud; (1) green valley; (3) red sequence: defined in equations (1) and (2).

Columns
-------
     1: ZIND(Byte) - redshift bin (0-4)
     2: MIND(Byte) - absolute magnitude bin (0-5)
     3: CIND(Byte) - colour bin (0-2)
     4: TOTFLUX(float[3]) - total stacked flux density (Jy/beam) at [250,350,500] microns
     5: TOTFERR(float[3]) - 
     6: CIBFRAC(float[3]) - TOTFLUX as a fraction of the Cosmic Infrared Background (see table 3)
     7: ECIBFRAC(float[3]) - 
     8: MEDFLUX(float[3]) - median stacked flux density (Jy/beam) at [250,350,500] microns
     9: MEDFERR_MEAS(float[3]) - measurement error on the median: instrumental+confusion noise
   10: MEDFERR_STAT(float[3]) - full statistical error on the median based on Gott et al. 2001
   11: MEDFLUXK(float[3]) - K-corrected median stacked flux density (Jy/beam)
   12: MEDFKERR(float[3]) - 
   13: MEDLUM(double[3]) - median monochromatic luminosity (W/Hz) at [250,350,500] microns (see figure 10)
   14: MEDLERR(double[3]) - 
   15: MEDC23(Float) - median 250/350 flux ratio (see figure 9)
   16: MEDC23ERR(Float) - 
   17: MEDC25(Float) - median 250/500 flux ratio (see figure 9)
   18: MEDC25ERR(Float) - 
   19: MEDC35(Float) - median 350/500 flux ratio (see figure 9)
   20: MEDC35ERR(Float) - 
   21: FITLDUST(Double) - best-fitting total dust luminosity in Smith+11b templates 
   22: FITLDERR(Float) - 
   23: MEDMDUST(Float) - dust mass derived from 250-micron luminosity with T=FITTDUST,beta=FITBETA (see figure 16)
   24: MEDMDUSTERR(Float) - 
   25: FITTPARAMS(float[4]) - parameters of the best fit for dust temperature [flux, T, beta]
   26: FITTDUST(Float) - best-fitting dust temperature (see figure 14)
   27: FITTERR(Float) - 
   28: FITBETA(Float) - best-fitting beta (actually fixed to 2.0 in this case)
   29: FITBERR(Float) - 
   30: MEDMDMS(Float) - median ratio of dust mass/stellar mass 
   31: MEDMDMSERR(Float) - 
   32: MEDZ(Float) - median redshift in the bin 
   33: MEDM(Float) - median absolute magnitude M_r in the bin
   34: MEDC(Float) - median g-r colour in the bin
   35: MLIMITS(float[2]) - [lower,upper] limits on M_r for the bin (redshift-dependent)
   36: MEDMSTAR(Float) - median stellar mass in the bin
   37: MEDMSTARERR(Float) - 
   38: MEDUVIR(Float) - median L_250/L_NUV ratio 
   39: MEDUVIRERR(Float) - 
   40: MED250R(Float) - median L_250/L_r ratio (not shown in paper)
   41: MED250RERR(Float) - 
   42: NBIN_NUV(Integer) - Number of galaxies in bin with NUV detection (contributing to Col 35,36)
   43: NBIN(Integer) - Total number of galaxies in bin
   44: KSTEST(float[3]) - KS test result for [250,350,500] micron flux distribution (see table 1)