060218 VLA 2006 Feb. 20.02 1.87 8.46 453 77 astro-ph/0604389 060218 VLA 2006 Feb. 20.02 1.87 4.86 127 81 astro-ph/0604389 060218 VLA 2006 Feb. 21.14 3.00 8.46 381 60 astro-ph/0604389 060218 VLA 2006 Feb. 21.14 3.00 22.5 250 52 astro-ph/0604389 060218 Ryle 2006 Feb. 21.17 3.62 15.0 350 350 astro-ph/0604389 060218 VLA 2006 Feb. 21.97 3.83 8.46 269 40 astro-ph/0604389 060218 VLA 2006 Feb. 21.97 3.83 4.86 287 56 astro-ph/0604389 060218 VLA 2006 Feb. 22.99 4.85 8.46 280 47 astro-ph/0604389 060218 VLA 2006 Feb. 22.99 4.85 4.86 328 61 astro-ph/0604389 060218 VLA 2006 Feb. 22.99 4.85 1.43 198 59 astro-ph/0604389 060218 VLA 2006 Feb. 25.12 6.97 4.86 80 47 astro-ph/0604389 060218 VLA 2006 Feb. 25.12 6.97 8.46 164 39 astro-ph/0604389 060218 VLA 2006 Feb. 25.12 6.97 1.43 134 145 astro-ph/0604389 060218 VLA 2006 Feb. 25.12 6.97 15.0 46 141 astro-ph/0604389 060218 VLA 2006 Feb. 26.09 7.94 8.46 30 30 astro-ph/0604389 060218 VLA 2006 Feb. 26.09 7.94 4.86 32 32 astro-ph/0604389 060218 VLA 2006 Feb. 28.10 9.95 8.46 39 25 astro-ph/0604389 060218 VLA 2006 Mar. 2.23 12.08 1.43 70 70 astro-ph/0604389 060218 VLA 2006 Mar. 3.03 12.88 8.46 15 15 astro-ph/0604389 060218 VLA 2006 Mar. 6.89 16.74 8.46 75 13 astro-ph/0604389 060218 VLA 2006 Mar. 10.01 19.86 8.46 48 14 astro-ph/0604389 060218 VLA 2006 Mar. 12.11 21.96 8.46 87 39 astro-ph/0604389 060218 VLA 2006 Mar. 15.04 24.91 8.46 20 20 astro-ph/0604389 060218 VLA 2006 Mar. 20.86 30.71 8.46 32 20 astro-ph/0604389 060218 VLA 2006 Mar. 24.96 34.81 8.46 15 18 astro-ph/0604389 060218 VLA 2006 Mar. 26.85 36.70 1.43 69 69 astro-ph/0604389 060218 VLA 2006 Mar. 26.85 36.70 4.86 5 37 astro-ph/0604389 060218 VLA 2006 Mar. 31.89 41.74 8.46 22 22 astro-ph/0604389 060218 VLA 2006 Apr. 9.84 50.70 8.46 25 22 astro-ph/0604389 These data are published in Soderberg et al. (Nature, submitted) 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".