. Author manuscript; available in PMC: 2020 Aug 26.

Published in final edited form as: Astrophys J. 2018 Aug 7;863(1):15. doi: 10.3847/1538-4357/aace62

Table 6.

Percentiles of the Expected Flux-density PDFs

Percentile	F(K) (mJy)	V_kLv_k (10³⁴ erg s ^{− 1})	F(M) (mJy)	V_MLv_M (10³⁴ erg s⁻¹)
5th	0.055	0.60	0.94	1.30
15th	0.110	1.19	1.49	2.06
25th	0.158	1.71	1.92	2.65
35th	0.208	2.26	2.33	3.21
45th	0.263	2.85	2.75	3.79
55th	0.325	3.52	3.19	4.40
65th	0.398	4.31	3.70	5.10
75th	0.489	5.29	4.33	5.98
85th	0.618	6.69	5.22	7.20
95th	0.877	9.49	6.94	9.57
99th	1.190	12.88	9.12	12.58

Note. Percentile flux densities for Case 3 (log-normal/log-normal parametrization). The luminosities were derived assuming a distance of the Galactic center of 8.3 kpc and extinctions A_K = 2.46 mag and A_M = 1.0 mag. The uncertainties of these quantities are not included in the calculations of expected luminosities.