GRB030329

	The GRB030329 Data Treasury - Plots

Selected plots and graphs

click on image for larger version	BVRI light curve of GRB 030329. Our observations are marked by circles, and the external data sets (see Table 1 in Lipkin et al. 2004), cross-calibrated to our photometric system, are marked by squares.
click on image for larger version	The binned B-R color of the OT during the first 40 days after the burst. The vertical axis on the right shows the corresponding spectral power-law, _BR. The inset is a blow-up of the first four days.
click on image for larger version	This plot is not presented in Lipkin et al. The binned V-I color of the OT during the first 14 days after the burst.
click on image for larger version	This plot is not presented in Lipkin et al. Smothed optical R-band light curve (dashed line) and Smothed SN- and host-subtracted R-band light curve (solid line) overlayed by the X-ray measurements presented by Tiengo et al.(2003), fitted by matching the measurement at day one. The arrow mark an upper limit observation.
click on image for larger version	This plot is not presented in Lipkin et al. The optical-to-radio spectral energy distribution (solid lines), in days 2.9, 4.8, 6.8 and 17.7 after the burst. The dashed line is the extrapolated optical to X-ray slope, and the extrapolated mm slope. The intersection points of these slopes are marked with circles.
click on image for larger version	This plot is not presented in Lipkin et al. The radio (15GHz) light curve of GRB 030329 (Berger et al. 2003)

Constructed: November 2003, Eran Ofek