The undetectable fraction of core-collapse supernovae in luminous infrared galaxies - II. GSAOI/GeMS dataset

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Table 1.

Summary of the dataset.

Galaxy	Na	tb	SFRc	t_SBd	CCSN ratee	L_AGNf	Dg	A_Gal, Kh
		(d)	(M_⊙ yr⁻¹)	(Myr)	(SN yr⁻¹)	(%)	(Mpc)	(mag)
ESO 264-G036	4	766	$76_{- 13}^{+ 9}$ $Mathematical equation: $ 76^{+9}_{-13} $$	$34_{- 2}^{+ 1}$ $Mathematical equation: $ 34^{+1}_{-2} $$	0.7 $_{- 0.1}^{+ 0.1}$ $Mathematical equation: $ ^{+0.1}_{-0.1} $$	19 $_{- 2}^{+ 5}$ $Mathematical equation: $ ^{+5}_{-2} $$	98.7	0.052
ESO 267-G030	4	1064	$22_{- 6}^{+ 12}$ $Mathematical equation: $ 22^{+12}_{-6} $$	$25_{- 4}^{+ 7}$ $Mathematical equation: $ 25^{+7}_{-4} $$	$0 . 2_{- 0.1}^{+ 0.1}$ $Mathematical equation: $ 0.2^{+0.1}_{-0.1} $$	$29_{- 3}^{+ 3}$ $Mathematical equation: $ 29^{+3}_{-3} $$	95.9	0.029
ESO 440-IG058	4	1116	$106_{- 4}^{+ 7}$ $Mathematical equation: $ 106^{+7}_{-4} $$	$36_{- 1}^{+ 1}$ $Mathematical equation: $ 36^{+1}_{-1} $$	$1 . 0_{- 0.1}^{+ 0.1}$ $Mathematical equation: $ 1.0^{+0.1}_{-0.1} $$	$18_{- 2}^{+ 5}$ $Mathematical equation: $ 18^{+5}_{-2} $$	110.6	0.023
IRAS 08355-4944	2	356	$45_{- 8}^{+ 2}$ $Mathematical equation: $ 45^{+2}_{-8} $$	$25_{- 2}^{+ 1}$ $Mathematical equation: $ 25^{+1}_{-2} $$	$0 . 6_{- 0.1}^{+ 0.1}$ $Mathematical equation: $ 0.6^{+0.1}_{-0.1} $$	$42_{- 2}^{+ 8}$ $Mathematical equation: $ 42^{+8}_{-2} $$	114.9	0.250
IRAS 17138-1017	6	801	$69_{- 4}^{+ 37}$ $Mathematical equation: $ 69^{+37}_{-4} $$	$28_{- 1}^{+ 7}$ $Mathematical equation: $ 28^{+7}_{-1} $$	0.8 $_{- 0.1}^{+ 0.1}$ $Mathematical equation: $ ^{+0.1}_{-0.1} $$	31 $_{- 4}^{+ 20}$ $Mathematical equation: $ ^{+20}_{-4} $$	82.2	0.207
IRAS 18293-3413	4	772	$275_{- 42}^{+ 50}$ $Mathematical equation: $ 275^{+50}_{-42} $$	$40_{- 5}^{+ 1}$ $Mathematical equation: $ 40^{+1}_{-5} $$	$2 . 3_{- 0.2}^{+ 0.4}$ $Mathematical equation: $ 2.3^{+0.4}_{-0.2} $$	$49_{- 9}^{+ 13}$ $Mathematical equation: $ 49^{+13}_{-9} $$	84.1	0.043
NGC 3110	4	408	$20_{- 5}^{+ 6}$ $Mathematical equation: $ 20^{+6}_{-5} $$	$20_{- 2}^{+ 6}$ $Mathematical equation: $ 20^{+6}_{-2} $$	$0 . 2_{- 0.1}^{+ 0.1}$ $Mathematical equation: $ 0.2^{+0.1}_{-0.1} $$	$30_{- 3}^{+ 3}$ $Mathematical equation: $ 30^{+3}_{-3} $$	77.9	0.011
NGC 3508	2	352	$8_{- 1}^{+ 1}$ $Mathematical equation: $ 8^{+1}_{-1} $$	$37_{- 2}^{+ 1}$ $Mathematical equation: $ 37^{+1}_{-2} $$	$0 . 1_{- 0.1}^{+ 0.1}$ $Mathematical equation: $ 0.1^{+0.1}_{-0.1} $$	$16_{- 2}^{+ 3}$ $Mathematical equation: $ 16^{+3}_{-2} $$	61.2	0.015
NGC 4575	2	353	$29_{- 3}^{+ 7}$ $Mathematical equation: $ 29^{+7}_{-3} $$	$35_{- 2}^{+ 3}$ $Mathematical equation: $ 35^{+3}_{-2} $$	$0 . 2_{- 0.1}^{+ 0.1}$ $Mathematical equation: $ 0.2^{+0.1}_{-0.1} $$	$10_{- 6}^{+ 3}$ $Mathematical equation: $ 10^{+3}_{-6} $$	62.6	0.037

Notes. The luminosity distances are corrected for the influence of the Virgo Cluster and the Great Attractor infall, and assumed H₀ = 70 km s⁻¹ Mpc⁻¹, Ω_M = 0.3, Ω_Λ = 0.7. The SFR, CCSN rate, and L_AGN values for IRAS 17138-1017 and IRAS 18293-3413 are adopted from Kankare et al. (2021). anumber of epochs, bsurvey coverage in days, cestimated SFR value, dstarburst age, eintrinsic rate of CCSNe, fAGN contribution to the luminosity, gluminosity distance, hGalactic line-of-sight extinction.

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