From kawabata@subaru.naoj.org Mon Mar 04 12:07:18 2002 I02ddCAL.xy : Flux data (dd=08, 09, 10, 11; obs date) They are scaled as the flux at 5550A corresponds to the CCD photometry by Lew Cook (VSNET). http://www.astr.tohoku.ac.jp/~kawabata/sn2002/VMAGEST.jpg I have not corrected for strong atmospheric absorption around 6900 and 7600A due to O_2 and interstellar absorption such as Na D. qupt02dd.xy : Polarization data (dd=08, 09, 10) They include lambda(A), q(%), u(%), P(%), theta(deg), Perr. The data are binned to a constant photon noise of Perr = 0.05 %. I ignore the spectropolarimetric data on Feb. 11 because they had much lower S/N than those on other days. quptmean.xy : Polarization data averaged over above three days. In this period, no significant change was seen in polarization properties as seen in the above plot. Data format is same as above files. The data are binned to a constant photon noise of Perr = 0.02 %. I have not corrected for the heliocentric redshift in these data. ************************************************** Perr must stand for photon noise error. I assume no reddening correction either NGC 628 = M74 heliocentric velocity from lines in sn spectra +631 km/s iauc 7822 S. Smartt & P. Meikle from Leda in radio +656 km/s from Leda in optical +639 km/s from Leda mean +656 km/s Foreground extinction in B from Leda/Schlegel 0.30 E(B-V)=.30/4 0.075 E(B-V)=.30/4.1 0.073 See Cardelli p. 249 Paolo E(B-V) 0.08 ********************************************** Polarization 2002 feb 9 lambda(A), q(%), u(%), P(%), theta(deg), Perr. END: 4751.5918 0.530799985 4832.20312 0.721599996 4901.56885 0.722000003 4963.69189 0.530200005 5019.4082 0.626299977 5075.06982 0.551699996 5123.52002 0.502300024 5165.33887 0.676699996 5206.93701 0.729200006 5248.50098 0.617299974 5290.18701 0.654500008 5324.85205 0.707099974 5352.66504 0.622399986 5380.45996 0.75819999 5408.20703 0.606599987 5436.00684 0.608200014 5463.76611 0.841300011 5491.56982 0.904100001 5519.3418 0.664499998 5547.1792 0.798399985 5574.95117 0.697099984 5609.55713 0.639699996 5651.27295 0.846599996 5693.13086 0.781000018 5734.9751 0.793299973 5776.65186 0.873700023 5818.3252 0.762000024 5859.96387 0.702000022 5901.67578 0.691999972 5943.26709 0.698499978 5985.05908 0.590399981 6026.61816 0.791199982 6068.47119 0.773699999 6110.20508 0.712499976 6151.7998 0.749800026 6193.72021 0.621999979 6235.43018 0.663699985 6277.06201 0.764699996 6311.78906 0.763400018 6339.5498 0.586600006 6367.30615 0.614700019 6395.08789 0.556599975 6422.90723 0.592000008 6450.69189 0.760299981 6478.521 0.752499998 6506.3042 0.671000004 6534.08203 0.76789999 6561.8999 0.809899986 6589.65381 0.756099999 6617.49707 0.666499972 6645.27295 0.679099977 6673.0708 0.662199974 6700.88086 0.844500005 6735.54102 0.644800007 6777.2041 0.726599991 6818.97412 0.803300023 6859.729 0.78549999 6902.80615 0.779999971 6944.18799 0.68720001 6985.75781 0.80309999 7027.47314 0.704200029 7069.13721 0.765200019 7110.94287 0.774999976 7152.45898 0.799099982 7194.32324 0.926500022 7235.74414 0.954599977 7284.3999 0.967400014 7339.69922 1.10230005 7401.30518 1.13129997 7477.70117 1.47570002 7569.29297 1.10080004 7686.62305 0.95630002 7764.87891 0.711199999 7826.92822 0.644200027 7882.43799 0.4903 7937.99219 0.457399994 7993.56885 0.412900001 8055.7002 0.328200012 8125.48193 0.700800002 8195.33105 0.592700005 8265.44141 0.634599984