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

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Table C.2

All SN Ia rate measurements used in this work.

z	Rate^a/ $10^{- 4} y r^{- 1} M p c^{- 3} h_{70}^{3}$ $/10^{-4} \mathrm{yr^{-1} Mpc^{-3} h^3_{70}}$	Reference
∼ 0	0.185 ± 0.05	(4)
0.14	${0.28}_{- 0.13 - 0.04}^{+ 0.22 + 0.07}$ $0.28^{+0.22+0.07}_{-0.13-0.04}$	(11)
0.098	0.24 ± 0.12	(14)
0.13	${0.158}_{- 0.043}^{+ 0.056} \pm 0.035$ $0.158^{+0.056}_{-0.043} \pm 0.035$	(2)
0.2-0.6	${0.69}_{- 0.27 - 0.25}^{+ 0.34 + 1.54}$ $0.69^{+0.34+1.54}_{-0.27-0.25}$	(6)
0.6-1.0	${1.57}_{- 0.25 - 0.53}^{+ 0.044 + 0.75}$ $1.57^{+0.044+0.75}_{-0.25-0.53}$	(6)
1.0-1.4	${1.15}_{- 0.26 - 0.44}^{+ 0.47 + 0.32}$ $1.15^{+0.47+0.32}_{-0.26-0.44}$	(6)
1.4-1.8	${0.44}_{- 0.25 - 0.11}^{+ 0.32 + 0.14}$ $0.44^{+0.32+0.14}_{-0.25-0.11}$	(6)
0.25	0.17 ± 0.17	(1)
0.3	${0.34}_{- 0.15 - 0.22}^{+ 0.16 + 0.21}$ $0.34^{+0.16+0.21}_{-0.15-0.22}$	(3)
0.09	${0.29}_{- 0.07}^{+ 0.09}$ $0.29^{+0.09}_{-0.07}$	(8)
0.2	${0.189}_{- 0.034 - 0.015}^{+ 0.042 + 0.018}$ $0.189^{+0.042+0.018}_{-0.034-0.015}$	(12)
0.025-0.050	${0.278}_{- 0.083 - 0.000}^{+ 0.112 + 0.015}$ $0.278^{+0.112+0.015}_{-0.083-0.000}$	(9)
0.075-0.125	${0.259}_{- 0.044 - 0.001}^{+ 0.052 + 0.018}$ $0.259^{+0.052+0.018}_{-0.044-0.001}$	(9)
0.125-0.175	${0.307}_{- 0.034 - 0.005}^{+ 0.038 + 0.035}$ $0.307^{+0.038+0.035}_{-0.034-0.005}$	(9)
0.175-0.225	${0.348}_{- 0.030 - 0.007}^{+ 0.032 + 0.082}$ $0.348^{+0.032+0.082}_{-0.030-0.007}$	(9)
0.225-0.275	${0.365}_{- 0.028 - 0.012}^{+ 0.031 + 0.182}$ $0.365^{+0.031+0.182}_{-0.028-0.012}$	(9)
0.275-0.325	${0.434}_{- 0.034 - 0.016}^{+ 0.037 + 0.396}$ $0.434^{+0.037+0.396}_{-0.034-0.016}$	(9)
∼ 0	0.301 ± 0.062	(13)
0.1-0.2	$0.14 \pm {0.09}_{- 0.12}^{+ 0.06}$ $0.14 \pm 0.09^{+0.06}_{-0.12}$	(16)
0.2-0.3	$0.28 \pm {0.07}_{- 0.07}^{+ 0.06}$ $0.28 \pm 0.07^{+0.06}_{-0.07}$	(16)
0.3-0.4	$0.36 \pm {0.06}_{- 0.06}^{+ 0.05}$ $0.36 \pm 0.06^{+0.05}_{-0.06}$	(16)
0.4-0.5	$0.36 \pm {0.06}_{- 0.05}^{+ 0.04}$ $0.36 \pm 0.06^{+0.04}_{-0.05}$	(16)
0.5-0.6	$0.48 \pm {0.06}_{- 0.05}^{+ 0.04}$ $0.48 \pm 0.06^{+0.04}_{-0.05}$	(16)
0.6-0.7	$0.48 \pm {0.05}_{- 0.06}^{+ 0.04}$ $0.48 \pm 0.05^{+0.04}_{-0.06}$	(16)
0.7-0.8	$0.58 \pm {0.06}_{- 0.07}^{+ 0.05}$ $0.58 \pm 0.06^{+0.05}_{-0.07}$	(16)
0.8-0.9	$0.57 \pm {0.05}_{- 0.07}^{+ 0.06}$ $0.57 \pm 0.05^{+0.06}_{-0.07}$	(16)
0.9-1.0	$0.77 \pm {0.08}_{- 0.12}^{+ 0.10}$ $0.77 \pm 0.08^{+0.10}_{-0.12}$	(16)
1.0-1.1	$0.74 \pm {0.12}_{- 0.13}^{+ 0.10}$ $0.74 \pm 0.12^{+0.10}_{-0.13}$	(16)
0.25	${0.36}_{- 0.26 - 0.35}^{+ 0.60 + 0.12}$ $0.36^{+0.60+0.12}_{-0.26-0.35}$	(17)
0.75	${0.51}_{- 0.19 - 0.19}^{+ 0.27 + 0.23}$ $0.51^{+0.27+0.23}_{-0.19-0.19}$	(17)
1.25	${0.64}_{- 0.22 - 0.23}^{+ 0.31 + 0.34}$ $0.64^{+0.31+0.34}_{-0.22-0.23}$	(17)
1.75	${0.72}_{- 0.30 - 0.28}^{+ 0.45 + 0.50}$ $0.72^{+0.45+0.50}_{-0.30-0.28}$	(17)
2.25	${0.49}_{- 0.38 - 0.24}^{+ 0.95 + 0.45}$ $0.49^{+0.95+0.45}_{-0.38-0.24}$	(17)
0.05-0.15	${0.55}_{- 0.29}^{+ 0.50} \pm 0.20$ $0.55^{+0.50}_{-0.29} \pm 0.20$	(5)
0.15-0.35	${0.39}_{- 0.12}^{+ 0.13} \pm 0.10$ $0.39^{+0.13}_{-0.12} \pm 0.10$	(5)
0.35-0.55	${0.52}_{- 0.13}^{+ 0.11} \pm 0.16$ $0.52^{+0.11}_{-0.13} \pm 0.16$	(5)
0.55-0.75	${0.69}_{- 0.18}^{+ 0.19} \pm 0.27$ $0.69^{+0.19}_{-0.18} \pm 0.27$	(5)
0.073	${0.243}_{- 0.029 - 0.019}^{+ 0.029 + 0.033}$ $0.243^{+0.029+0.033}_{-0.029-0.019}$	(10)
<0.1	0.235 ± 0.024	(15)
0.01-0.04	${0.291}_{- 0.045}^{+ 0.058}$ $0.291^{+0.058}_{-0.045}$	(18)
0.024	0.228 ± 0.020	(7)
0-0.01	$0.325 \pm {0.040}_{- 0.010}^{+ 0.016}$ $0.325 \pm 0.040^{+0.016}_{-0.010}$	this work

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

References. (1) Barris & Tonry (2006); (2) Blanc et al. (2004); (3) Botticella et al. (2008); (4) Cappellaro et al. (1999); (5) Cappellaro et al. (2015); (6) Dahlen et al. (2004); (7) Desai et al. (2024); (8) Dilday et al. (2008); (9) Dilday et al. (2010); (10) Frohmaier et al. (2019); (11) Hardin et al. (2000); (12) Horesh et al. (2008); (13) Li et al. (2011a); (14) Madgwick et al. (2003); (15) Perley et al. (2020); (16) Perrett et al. (2012); (17) Rodney et al. (2014); (18) Sharon & Kushnir (2022).

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