Supernovae at distances <40 Mpc - II. Supernova rate in the local Universe

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Table C.1

All CCSN rate measurements used in this work.

z	Rate $^{a} / 10^{- 4} y r^{- 1} M p c^{- 3} h_{70}^{3}$ $^{a}/10^{-4} \mathrm{yr^{-1} Mpc^{-3} h^3_{70}}$	Reference
0.1-0.5	${2.51}_{- 0.75 - 1.86}^{+ 0.88 + 0.75}$ $2.51^{+0.88+0.75}_{-0.75-1.86}$	(6)
0.5-0.9	${3.96}_{- 1.06 - 2.60}^{+ 1.03 + 1.92}$ $3.96^{+1.03+1.92}_{-1.06-2.60}$	(6)
0.26	${1.789}_{- 0.57}^{+ 0.65}$ $1.789^{+0.65}_{-0.57}$	(4)
0.21	${1.15}_{- 0.33 - 0.36}^{+ 0.43 + 0.42}$ $1.15^{+0.43+0.42}_{-0.33-0.36}$	(2)
0.3	$1.63 \pm {0.30}_{- 0.24}^{+ 0.32}$ $1.63 \pm 0.30^{+0.32}_{-0.24}$	(1)
∼ 0	0.705 ± 0.211	(10)
0.003	1.626 ± 0.407	(3)
0.39	${3.00}_{- 0.94 - 0.57}^{+ 1.28 + 1.04}$ $3.00^{+1.28+1.04}_{-0.94-0.57}$	(7)
0.73	${7.39}_{- 1.52 - 1.60}^{+ 1.86 + 3.20}$ $7.39^{+1.86+3.20}_{-1.52-1.60}$	(7)
1.11	${9.57}_{- 2.80 - 2.80}^{+ 3.76 + 4.96}$ $9.57^{+3.76+4.96}_{-2.80-2.80}$	(7)
0.39	${3.29}_{- 1.78 - 1.45}^{+ 3.08 + 1.98}$ $3.29^{+3.08+1.98}_{-1.78-1.45}$	(11)
0.73	${6.40}_{- 3.12 - 2.11}^{+ 5.30 + 3.65}$ $6.40^{+5.30+3.65}_{-3.12-2.11}$	(11)
0.072	1.06 ± 0.11 ± 0.15	(13)
0.075	${1.04}_{- 0.26 - 0.11}^{+ 0.33 + 0.04}$ $1.04^{+0.33+0.04}_{-0.26-0.11}$	(9)
0.05-0.15	${1.13}_{- 0.53 - 0.49}^{+ 0.62 + 0.49}$ $1.13^{+0.62+0.49}_{-0.53-0.49}$	(5)
0.15-0.35	1.21 ± 0.27 ± 0.47	(5)
0.1-0.5	${1.97}_{- 0.85}^{+ 1.45}$ $1.97^{+1.45}_{-0.85}$	(12)
0.5-0.9	${2.68}_{- 1.04}^{+ 1.54}$ $2.68^{+1.54}_{-1.04}$	(12)
0.9-1.3	${1.70}_{- 0.71}^{+ 1.19}$ $1.70^{+1.19}_{-0.71}$	(12)
1.3-1.7	${3.25}_{- 1.32}^{+ 2.03}$ $3.25^{+2.03}_{-1.32}$	(12)
1.7-2.1	${3.16}_{- 1.77}^{+ 3.37}$ $3.16^{+3.37}_{-1.77}$	(12)
2.1-2.5	${6.17}_{- 3.52}^{+ 6.76}$ $6.17^{+6.76}_{-3.52}$	(12)
0.028	${0.910}_{- 0.127}^{+ 0.156}$ $0.910^{+0.156}_{-0.127}$	(8)
0-0.01	$0.688 \pm {0.078}_{- 0.027}^{+ 0.206}$ $0.688 \pm 0.078^{+0.206}_{-0.027}$	this work

Notes. ^(a) Uncertainty is split between statistical and systematic uncertainty.

References. (1) Bazin et al. (2009); (2) Botticella et al. (2008); (3) Botticella et al. (2012); (4) Cappellaro et al. (2005); (5) Cappellaro et al. (2015); (6) Dahlen et al. (2004); (7) Dahlen et al. (2012); (8) Frohmaier et al. (2021); (9) Graur et al. (2015); (10) Li et al. (2011a); (11) Melinder et al. (2012); (12) Strolger et al. (2015); (13) Taylor et al. (2014).

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