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Table A.1

Optical photometry of three CCCP long-rising SNe II.

JD2 400 000 B V R/unf. I
(days) (mag) (mag) (mag) (mag)

SN 2004ek
53 263.47* 16.870(0.030) 16.770(0.030) 16.610(0.020) 16.380(0.040)
53 267.20 17.105(0.016) 16.866(0.018) 16.622(0.007) 16.277(0.032)
53 269.41* 17.060(0.030) 16.900(0.040) 16.570(0.040) 16.300(0.050)
53 272.17 17.305(0.016) 16.966(0.019) 16.712(0.010) 16.258(0.033)
53 276.18 17.505(0.038) 17.036(0.030) 16.723(0.010) 16.358(0.037)
53 280.24 17.495(0.016) 17.066(0.020) 16.742(0.009) 16.308(0.032)
53 282.16 ... ... ... 16.328(0.033)
53 283.40 17.525(0.016) 17.116(0.019) 16.782(0.007) 16.328(0.033)
53 288.22 17.485(0.019) ... 16.663(0.018) 16.238(0.034)
53 290.41 ... 17.116(0.066) ... ...
53 292.17 17.515(0.020) ... 16.642(0.010) ...
53 294.26* 17.570(0.030) 17.030(0.030) 16.610(0.030) 16.250(0.030)
53 302.18 17.555(0.025) 17.016(0.021) ... ...
53 303.46 17.525(0.019) 16.966(0.027) 16.492(0.007) 16.117(0.037)
53 307.41* 17.620(0.060) 16.960(0.040) 16.490(0.030) 16.040(0.030)
53 308.37 17.595(0.070) ... ... ...
53 310.24 ... 16.896(0.023) 16.483(0.015) 16.087(0.044)
53 312.51* 17.520(0.040) 16.870(0.030) 16.430(0.030) 16.070(0.030)
53 313.24 ... 16.876(0.018) ... 16.008(0.033)
53 315.45* 17.500(0.040) 16.860(0.020) 16.430(0.020) 16.050(0.050)
53 316.24 17.505(0.019) 16.856(0.021) 16.363(0.007) 15.998(0.032)
53 317.30* 17.650(0.030) 16.780(0.020) 16.500(0.020) 16.090(0.050)
53 318.50* 17.580(0.040) 16.790(0.030) 16.370(0.040) ...
53 320.45* 17.53 0(0.020) 16.890(0.020) 16.420(0.020) 16.040(0.040)
53 321.47* 17.640(0.030) 16.820(0.020) 16.310(0.010) 15.950(0.040)
53 322.17 17.595(0.018) 16.856(0.019) 16.392(0.007) 15.967(0.033)
53 323.49* 17.570(0.030) 16.870(0.020) 16.350(0.020) 15.950(0.030)
53 325.26 17.605(0.015) 16.906(0.018) 16.402(0.006) ...
53 328.35 17.645(0.015) ... ... 15.957(0.032)
53 329.25 ... 16.856(0.019) 16.363(0.007) ...
53 331.47* 17.650(0.040) 16.840(0.020) 16.360(0.020) 15.930(0.030)
53 335.16 ... 16.906(0.027) 16.312(0.026) ...
53 383.27* 18.790(0.180) ... 16.760(0.040) ...
53 386.12 18.995(0.051) 17.776(0.029) 16.992(0.014) 16.317(0.046)
53 389.37* ... 17.400(0.200) ... ...
53 405.22* ... 17.840(0.140) 17.070(0.070) ...
53 412.26* ... 17.710(0.190) 17.190(0.140) ...
53 538.45 ... 21.006(0.657) 19.973(0.091) 19.087(0.540)
53 539.41 ... ... 20.023(0.122) ...

SN 2004em
53 276.17 17.870(0.082) 17.647(0.055) 17.503(0.079) 17.382(0.073)
53 279.14 17.930(0.074) 17.647(0.060) 17.483(0.126) 17.432(0.081)
53 281.13 17.900(0.074) 17.577(0.058) 17.353 (0.032) 17.082(0.064)
53 284.14 18.140(0.075) 17.617(0.054) 17.453 (0.104) 17.252(0.059)
53 287.10 ... ... 17.303(0.053 ) ...
53 289.17 18.270(0.112) 17.607(0.057) ... 16.872(0.071)
53 292.12 18.170(0.077) 17.547(0.074) 17.403(0.026) 17.042(0.054)
53 302.17 18.560(0.086) 17.707(0.066) 17.453 (0.039) 17.172(0.069)
53 309.11 18.630(0.079) 17.677(0.057) 17.383(0.031) 17.172(0.082)
53 310.18 18.550(0.113) 17.667(0.106) 17.403(0.072) 17.052(0.155)
53 322.11 ... 17.387(0.054) ... ...
53 324.11 ... ... ... 16.592(0.081)
53 329.14 18.210(0.079) 17.117(0.054) 17.013(0.041) 16.682(0.046)
53 334.14 ... ... 16.713(0.151) 16.542(0.088)
53 351.14 ... ... 16.593(0.035) ...
53 352.11 17.830(0.073) 16.897(0.053 ) 16.583(0.020) 16.402(0.068)
53 401.55 ... 17.127(0.154) 16.753 (0.179) 16.312(0.106)
53 405.56 ... 17.297(0.069) ... ...
53 406.54 ... ... 16.943(0.054) 16.662(0.065)
53 537.32 ... ... 19.453 (0.717) ...
53 538.37 ... 20.296(0.153) 19.543(0.689) 20.362(0.983)

SN 2005ci
53 523.86** ... ... 20.160(0.150) ...
53 531.81** ... ... 18.780(0.130) ...
53 532.85** ... ... 18.750(0.130) ...
53 533.83** ... ... 18.760(0.130) ...
53 534.76** ... ... 18.860(0.130) ...
53 535.18 19.340(0.299) ... 18.742(0.107) 18.417(0.329)
53 536.21 19.480(0.280) ... 18.662(0.152) 18.117(0.383)
53 536.80** ... ... 18.510(0.160) ...
53 539.23 ... 19.052(0.138) ... 17.877(0.417)
53 540.82** ... ... 18.310(0.130) ...
53 544.26 19.540(0.482) 18.702(0.188) 18.152(0.071) 17.527(0.214)
53 545.79** ... ... 18.180(0.130) ...
53 546.28 19.610(0.182) 18.432(0.186) 17.992(0.079) 17.377(0.259)
53 548.23 19.380(0.277) 18.322(0.177) 17.982(0.049) 17.417(0.258)
53 549.78** ... ... 17.940(0.130) ...
53 550.18 19.000(0.233) ... 17.822(0.026) 17.087(0.191)
53 552.34 ... 18.172(0.156) 17.632(0.050) ...
53 553.79** ... ... 17.750(0.130) ...
53 554.41 18.870(0.244) 18.112(0.133) 17.452(0.037) ...
53 557.30 19.000(0.227) ... ... 16.987(0.152)
53 557.78** ... ... 17.630(0.130) ...
53 559.22 19.010(0.192) 17.972(0.115) ... 16.967(0.115)
53 560.26 19.070(0.181) 17.822(0.107) 17.422(0.047) 16.847(0.138)
53 561.76** ... ... 17.720(0.150) ...
53 562.18 19.160(0.222) 17.982(0.127) 17.472(0.028) 16.847(0.133)
53 563.30 19.000(0.190) 17.972(0.072) ... 16.747(0.110)
53 565.75** ... ... 17.530(0.130) ...
53 567.68** ... ... 17.680(0.150) ...
53 570.19 18.990(0.245) 17.682(0.113) 17.262(0.033) 16.597(0.116)
53 573.30 ... 17.762(0.134) 17.222(0.051) 16.477(0.113)
53 581.29 18.990(0.212) 17.612(0.103) 17.162(0.043) 16.387(0.107)
53 587.24 18.970(0.251) 17.632(0.099) 17.012(0.036) 16.407(0.113)
53 590.29 18.770(0.192) 17.572(0.094) ... 16.287(0.093)
53 595.16 ... 17.522(0.091) ... 16.137(0.149)
53 600.21 18.840(0.129) 17.452(0.075) 16.922(0.035) 16.177(0.097)
53 602.18 18.990(0.493) 17.422(0.073) 16.802(0.033) 16.137(0.098)
53 611.93 18.760(0.139) 17.422(0.074) 16.792(0.028) 16.177(0.103)
53 613.23 18.930(0.215) 17.442(0.103) ... 16.077(0.100)
53 614.24 ... ... 16.782(0.023) ...
53 615.17 18.720(0.152) 17.422(0.093) ... 16.127(0.116)
53 616.21 18.840(0.252) 17.472(0.098) 16.802(0.033) 16.097(0.102)
53 619.16 18.900(0.197) 17.462(0.082) ... 16.147(0.103)
53 620.18 ... 17.552(0.056) ... 16.117(0.174)
53 621.19 ... 17.492(0.092) ... 16.157(0.107)
53 623.23 ... ... 16.822(0.047) ...
53 628.20 18.920(0.476) ... ... 16.037(0.125)
53 632.13 19.260(0.356) 17.842(0.203) 17.102(0.033) ...
53 643.11 19.240(0.655) 18.332(0.203) 17.532(0.084) 16.787(0.157)
53 649.15 ... 18.612(0.297) 17.842(0.074) ...
53 653.11 19.740(0.430) 19.072(0.349) 17.932(0.078) 17.137(0.202)

Notes. Besides CCCP photometry from Arcavi et al. (2012), the table includes BVRI photometry from Tsvetkov (2008) (marked by “*” and shifted by +0.1 (B), +0.2(V), +0.2(R), and +0.1(I) mag with respect to the original values of Tsvetkov 2008 to match the CCCP photometry) of SN 2004ek and unfiltered photometry of SN 2005ci from Kleiser et al. (2011) (marked by “**”).

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