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Table 2.

Type Ibc broad sample.

SN Type RA Dec z DM E(B − V)MW E(B − V)host Max epoch Exp. epoch sr sg
(deg) (deg) (mag) (mag) (mag) (JD) (JD)
PTF09dfk Ib 347.30593 7.80429 0.016 34.20 0.0458 0.28 ± 0.07 2455096.39 2455053.8 ± 1.3 2.36 ± 0.08 ...
PTF10inj Ib 238.73781 53.77195 0.064 37.34 0.0100 0.20 ± 0.12 2455378.22 2455339.9 ± 0.5 1.91 ± 0.06 2.17 ± 0.04
PTF11bov Ic 194.22475 22.37448 0.022 34.90 0.0289 0.06 ± 0.02 2455682.97 2455645.0 ± 0.5 2.04 ± 0.05 2.23 ± 0.08
PTF11mnb Ic 8.55522 2.80873 0.060 37.15 0.0157 0.06 ± 0.01 2455860.18 2455802.2 ± 1.2 2.46 ± 0.16 1.54 ± 0.12
PTF11rka Ic 190.18696 12.88927 0.074 37.63 0.0295 0.21 ± 0.05 2455932.87 2455896.0 ± 8.8 2.16 ± 0.09 ...
iPTF15dtg Ic 37.58355 37.23519 0.052 36.84 0.0549 ∼0 2457368.64 2457330.2 ± 0.4 2.07 ± 0.01 1.76 ± 0.16
iPTF16flq Ic 7.15223 −1.55092 0.060 37.14 0.0190 ∼0 2457647.67 2457616.1 ± 2.2 2.03 ± 0.10 2.21 ± 0.17
iPTF16hgp Ic 3.02672 32.19747 0.081 37.77 0.0382 0.06 ± 0.01 2457710.99 2457679.7 ± 0.5 1.83 ± 0.12 1.51 ± 0.05

Notes. Epoch of maximum light is estimated from r-band template fits. Explosion epoch is estimated in Sect. 5.1 via Arnett model fits. The stretch parameter in each band, i.e., the broadness of the lightcurve compared to a template, is also reported as measured in Appendix A.3. The host extinction estimate is derived in Sect. 3.4.

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