Table 2: Log of GMRT observations of GRB 030329.
Observing Dates $\Delta$T Frequency Fluxa
  (days) (MHz) (mJy)
2004 Jan. 4.97 281.49 610 $0.90\pm 0.20$
2004 Feb. 26.63 334.15 610 $1.14\pm 0.25$
2004 Apr. 10.49 378.01 610 $0.61\pm 0.11$
2004 Jun. 27.28 455.80 610 $1.01\pm 0.18$
2004 Jun. 28.28 456.80 1280 $1.11\pm 0.13$
2004 Jul. 18.31 476.83 1280 $1.04\pm 0.11$
2004 Jul. 20.28 478.80 610 $0.84\pm 0.17$
2004 Aug. 20.04 509.56 1280 $1.03\pm 0.11$
2004 Sep. 06.00 526.52 610 $0.98\pm 0.15$
2004 Sep. 17.96 538.48 1280 $0.48\pm 0.10$
2004 Dec. 3.00 614.52 610 $1.08\pm 0.35$
2005 Jan. 6.82 649.34 610 $0.50\pm 0.11$
2005 Feb. 8.81 682.33 325 < $1.5 (3\sigma)$b
2005 Feb. 13.84 687.34 1280 $0.97\pm 0.14$
2005 Feb. 21.71 695.23 610 $0.47\pm 0.13$
2005 Mar. 10.77 712.29 1280 $0.72\pm 0.07$
2005 Mar. 18.66 720.18 610 $0.69\pm 0.13$
2005 Jun. 17.54 811.06 610 < $1.1 (3\sigma)$c
2005 Jun. 28.59 702.11 325 < $1.8 (3\sigma)^b$
2005 Jul. 1.19 824.71 1280 $0.53\pm 0.09$
2005 Sep. 2.99 888.51 610 $0.68\pm 0.13$
2005 Oct. 8.20 923.72 1280 $0.49\pm 0.09$
a The measurement uncertainties are given at $1 \sigma$ level.
b A meaningful formal flux measurement at the GRB position cannot be determined
because of confusion by a very nearby, bright source.
c Formal flux measurement at the GRB position gives $0.74\pm 0.36$ mJy.

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