030226    VLA   2003 Feb. 26.28  0.12   8.46    -58     74        xxxxxx
030226    Ryle  2003 Feb. 27.10  0.94   15.0    190     220       xxxxxx
030226    VLA   2003 Feb. 27.25  1.09   8.46     70     12        xxxxxx
030226    OVRO  2003 Feb. 28.43  2.27   98.0    -99     600       xxxxxx
030226    VLA   2003 Mar. 01.36  3.20   22.5    104     47        xxxxxx
030226    VLA   2003 Mar. 02.26  4.10   8.46    131     27        xxxxxx
030226    VLA   2003 Mar. 08.38 10.20   22.5    137     59        xxxxxx
030226    VLA   2003 Mar. 09.27 11.11   8.46    121     27        xxxxxx
030226    VLA   2003 Mar. 10.41 12.25   22.5    328     74        xxxxxx
030226    VLA   2003 Mar. 14.40 16.24   8.46     44     37        xxxxxx
030226    VLA   2003 Mar. 15.33 17.17   22.5    227     66        xxxxxx
030226    VLA   2003 Mar. 17.44 19.28   8.46    5.2     23        xxxxxx
030226    VLA   2003 Mar. 20.35 22.19   8.46     40     21        xxxxxx
030226    VLA   2003 Mar. 23.19 25.03   8.46     35     18        xxxxxx
030226    VLA   2003 Jun. 20.01 113.85  1.43     27     39        xxxxxx

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".