050525A   VLA   2005 May  25.44  0.44   4.86     97      49       xxxxxxx
050525A   VLA   2005 May  25.44  0.44   8.46     80      34       xxxxxxx
050525A   VLA   2005 May  25.42  0.42   22.5    558      81       gcn3495
050525A   VLA   2005 May  26.36  1.36   8.46    -99      49       xxxxxxx
050525A   VLA   2005 May  26.36  1.36   22.5    422     108       gcn3495
050525A   VLA   2005 May  28.33  3.33   8.46    164      46       xxxxxxx
050525A   VLA   2005 May  31.45  6.45   8.46    -99      54       xxxxxxx
050525A   VLA   2005 May  31.45  6.45   22.5    115     176       xxxxxxx
050525A   VLA   2005 Jun.  7.47 13.47   4.86    143      82       xxxxxxx
050525A   VLA   2005 Jun.  7.47 13.47   8.46    164      48       xxxxxxx
050525A   VLA   2005 Jun.  7.47 13.47   22.5    -99     164       xxxxxxx
050525A   VLA   2005 Jun. 13.44 19.44   1.43    -99     206       xxxxxxx
050525A   VLA   2005 Jun. 13.44 19.44   4.86    -99      64       xxxxxxx
050525A   VLA   2005 Jun. 13.44 19.44   8.46     88      42       xxxxxxx
050525A   VLA   2005 Jun. 17.54 23.54   4.86     91      54       xxxxxxx
050525A   VLA   2005 Jun. 17.54 23.54   8.46     56      59       xxxxxxx
050525A   VLA   2005 Jun. 26.47 32.47   8.46    178      46       xxxxxxx
050525A   VLA   2005 Jun. 28.48 34.48   4.86    152      52       xxxxxxx
050525A   VLA   2005 Jun. 28.48 34.48   8.46    -99      40       xxxxxxx
050525A   VLA   2005 Jul.  2.52 38.52   8.46    -99      39       xxxxxxx


The entries in this file (from left to right) are the GRB name, the
radio telescope used to carry out the observation, the UT date of the
observation (usually taken at the midpoint of the integration), the
time since the burst in days, the observing frequency in GHz, the flux
density, the rms noise, and a reference noting where the data were
published. For those cases where no flux density measurements were
made, the flux density column contains "-99".