050904    VLA   2005 Sep.  4.58   0.50  8.46    89      59        xxxxxxx
050904    VLA   2005 Sep.  5.48   1.40  8.46    38      28        xxxxxxx
050904    VLA   2005 Sep.  9.48   5.40  8.46    -4      32        xxxxxxx
050904    VLA   2005 Sep. 10.31   6.23  8.46     8      38        xxxxxxx
050904    VLA   2005 Sep. 24.20  20.12  8.46   111      51        xxxxxxx
050904    VLA   2005 Oct.  3.36  29.28  8.46    76      32        xxxxxxx
050904    VLA   2005 Oct.  7.30  33.22  8.46    10      47        xxxxxxx
050904    VLA   2005 Oct.  8.26  34.18  8.46   108      31        xxxxxxx
050904    VLA   2005 Oct.  9.34  35.26  8.46    86      30        xxxxxxx
050904    VLA   2005 Oct. 11.43  37.35  8.46    41      21        xxxxxxx
050904    VLA   2005 Oct. 18.37  44.29  8.46    18      38        xxxxxxx

Needs re-processing and better self-cal.

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".