Four GRB supernovae at redshifts between 0.4 and 0.8 - The bursts GRB 071112C, 111228A, 120714B, and 130831A

S. Klose; S. Schmidl; D. A. Kann; A. Nicuesa Guelbenzu; S. Schulze; J. Greiner; F. Olivares E.; T. Krühler; P. Schady; P. M. J. Afonso; R. Filgas; J. P. U. Fynbo; A. Rau; A. Rossi; K. Takats; M. Tanga; A. C. Updike; K. Varela

doi:10.1051/0004-6361/201832728

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Volume 622 (February 2019)

A&A, 622 (2019) A138

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Table C.1.

Summary of the measured supernova parameters.

GRB	071112C	111228A	120714B	130831A
k_g′	...	...	...	0.87 ± 0.24
k_r′	0.53 ± 0.17	0.63 ± 0.14	0.47 ± 0.05	0.61 ± 0.04
k_i′	0.70 ± 0.17	0.73 ± 0.15	0.74 ± 0.06	0.99 ± 0.05
k_z′	0.52 ± 0.21	0.85 ± 0.27	0.78 ± 0.08	0.58 ± 0.12
s_g′	...	...	...	0.64 ± 0.09
s_r′	0.75 ± 0.19	1.58 ± 0.23	0.66 ± 0.04	0.80 ± 0.02
s_i′	0.78 ± 0.23	1.20 ± 0.25	0.91 ± 0.06	0.72 ± 0.02
s_z′	0.71 ± 0.35	1.45 ± 0.25	0.95 ± 0.09	0.72 ± 0.07
t_{g′,obs, p} (days)	...	...	...	13.7 ± 2.5
t_{r′,obs, p}	23.1 ± 6.6	45.8 ± 9.1	15.6 ± 2.3	20.0 ± 2.8
t_{i′,obs, p}	26.2 ± 8.7	37.9 ± 9.8	23.4 ± 4.9	19.6 ± 3.0
t_{z′,obs, p}	24.7 ± 12.8	47.5 ± 11.3	25.4 ± 5.9	20.3 ± 3.8
t_{g′,obs, p}	...	...	...	9.3 ± 1.7
t_{r′,obs, p}	12.7 ± 3.6	26.7 ± 5.3	11.2 ± 1.7	13.5 ± 1.9
t_{i′,obs, p}	14.4 ± 4.8	22.1 ± 5.7	16.7 ± 2.8	13.2 ± 2.0
t_{z′,obs, p}	13.6 ± 7.0	27.7 ± 6.6	18.1 ± 3.4	13.8 ± 2.6
log L_bol (erg s⁻¹)	42.73 ± 0.08	42.83 ± 0.09	42.79 ± 0.05	42.84 ± 0.05
t_p (days)	11.9 ± 2.4	22.7 ± 2.2	13.6 ± 0.7	11.9 ± 0.3
v_exp; obs (km s⁻¹)	...	...	43 000 ± 5300	20 400 ± 3500
v_exp; peak	...	...	42 000 ± 5500	30 300 ± 6000

Notes. The first eight rows summarize the measured (s, k) values in the GROND g′r′i′z′ bands. The following rows contain the corresponding SN peak times in the observer as well as in the host galaxy frame, t_p(SN) = t_p(SN 1998bw) × s. Thereby we used the light-curve peak times for SN 1998bw as they follow from our SN fitting procedure (Zeh et al. 2004): t_p(g′) = 14.5 ± 1.7, t_p(r′) = 16.9 ± 2.3, t_p(i′) = 18.4 ± 2.8, t_p(z′) = 19.1 ± 3.1 days. The following two rows provide the bolometric luminosity, , as well as the bolometric light-curve peak time (given by , with days; Prentice et al. 2016). The two last rows list the photospheric expansion velocity as it was measured and its calculated value for the time of the peak of the bolometric light curve.

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