RUNZ training fields
====================

Setup by Karl Glazebrook (Created 23rd Aug, 2007)

Three fields, redshifted by experts. (Named in the header.)

Use runz and select "u - use old redshifts, and start again". Step
through in review mode by pressing the '0' key. (If you exit with Ctrl-C you
will not overwrite the old file). Or make a copy and try and redshift yourself.

The most critical thing to pay attention to is the Q=2 to Q=3 boundary. The 
Q=4/5 boundary is also fuzzy (a matter of opinion) but less important.

Here are the statistics:


                        Total |         Number with QOP=    |       percentage with QOP=         |  percent QOP>2
    field name          Number|   0   1   2   3   4   5   6 |   0    1    2    3    4    5    6  |   all z  z>0.5
--------------------------------------------------------------------------------------------------------------
r00f21s01_070814_BR_ssz.rz 328 |  12 106  24  75  94  17   0 |  3.7 32.3  7.3 22.9 28.7  5.2  0.0 |    56.7   40.2  
r15f34s01_070809_BR_ssz.rz 336 |   0   7  55  91 146  37   0 |  0.0  2.1 16.4 27.1 43.5 11.0  0.0 |    81.5   56.8  
r22f06s01_070811_BR_ssz.rz 337 |   0  36  16  28 236  18   3 |  0.0 10.7  4.7  8.3 70.0  5.3  0.9 |    84.6   41.5  

So two of the fields have very high completeness to make it easy for you! 
The other is a difficult, low completeness field which unfortunately is not
uncommon.

DON'T JUST LOOK AT THE 22h FIELD!!! It is one of the best and contains an 
unusually low fraction of Q=3 objects.

Note any object with R<20 is an RCS2 target, quite often an absorption line 
galaxy and usually easy. Pay attention to the features.

