IMPORTANT:  Note that first column shows high priority (*) objects
and those targets for which we already have a spectrum (S).


      ID#    RA           Dec           Epoch    mag  Offset from host?
                                                       
*  1 9570    00:26:29.40  +07:34:45.33   1950    22.4    o
   2 9571    00:56:08.69  +06:02:11.72   1950    22.0    A
S  3 9579    00:58:45.38  +04:02:25.86   1950    23.0    o
S  4 9569    00:59:00.23  +04:10:07.19   1950    23.2    o
*  5 95116   01:02:15.76  +04:17:49.25   1950    22.7    o
S  6 9591    01:59:00.93  +03:24:28.09   1950    20.1    A 
   7 9568    02:22:21.25  +00:39:35.89   1950    22.4    A
   8 95115   02:22:23.93  +00:26:44.41   1950    22.4  faint host
S  9 95126   02:23:51.56  +00:35:16.36   1950    22.6    o
* 10 95104   02:58:33.55  +00:09:30.31   1950    22.7    o
S"13" 95103  04:38:05.93  -05:35:49.09   1950    23.4    o
S 11 95110   08:16:25.17  +07:52:47.93   1950    22.6    o



  SN found in one-year baseline -- now on the way down:
  12 9528    01:15:55.82  +07:38:17.81   1950    21.7    o

Faint ones we are still confirming, if possible:


______________________________________________________________________________
* = highest priority -- needs spectrum
S = spectrum already obtained 
______________________________________________________________________________

______________________________________________________________________________
o = off center of host galaxy
A = on  center of host galaxy
______________________________________________________________________________