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Table 1

Input parameters for the photoionization models.

Parameter Values
JY20 model (fiducial model in this work, Ji & Yan 2020)

log(U) − 4.0, − 3.75, − 3.5, − 3.25, − 3.0, − 2.75, − 2.5, − 2.25, − 2.0, − 1.75, − 1.5
log(ZZ) − 1.3, − 0.7, − 0.4, 0.0, 0.3, 0.5
log(nH∕cm−3) 1.15
Geometry Plane-parallel
Stellar SED STARBURST99 model with a continuous SFH of 4 Myr
Solar abundance set Grevesse et al. (2010) solar abundance set
Nitrogen prescription Dopita et al. (2013) prescription
Depletion factor Default depletion set in CLOUDY (Cowie & Songaila 1986; Jenkins 1987)

L10 model (Levesque et al. 2010)

log(U) − 3.5, − 3.2, − 2.9, − 2.6, − 2.5, − 2.2, − 1.9
log(Z/Z) − 1.3, − 0.7, − 0.4, 0.0, 0.3
log(nH∕cm−3) 2.0
Geometry Plane-parallel
Stellar SED STARBURST99 model with a continuous SFH of 6 Myr
Solar abundance set Anders & Grevesse (1989) solar abundance set (E. Levesque, priv. comm.)
Nitrogen prescription Unspecified
Depletion factor Unspecified

D13 model (κ, Dopita et al. 2013)

log(U) − 4.0, − 3.7, − 3.5, − 3.2, − 3.0, − 2.7, − 2.5, − 2.2, − 2.0
log(ZZ) − 1.3, − 1.0, − 0.7, − 0.5, − 0.3, 0.0, 0.3, 0.5, 0.7
log(nH∕cm−3) 1.0
Geometry Spherical
Stellar SED (Old) STARBURST99 model with a continuous SFH of 4 Myr (see Dopita et al. 2000)
Solar abundance set Grevesse et al. (2010) solar abundance set
Nitrogen prescription Dopita et al. (2013) prescription
Depletion factor Depletion set described in Kimura et al. (2003) and Dopita et al. (2005)

B17 model (extracted from PYTHON-FSPS, Byler et al. 2017)

log(U) − 4.0, − 3.5, − 3.0, − 2.5, − 2.0, − 1.5, − 1.0
log (ZZ) − 2.0, − 1.5, − 1.0, − 0.6, − 0.4, − 0.3, − 0.2, − 0.1, 0.0, 0.1, 0.2
log (nH ∕cm−3) 2.0
Geometry Spherical
Stellar SED FSPS model with an instantaneous SFH of 1 Myr
(MIST evolutionary track, see Dotter 2016 and Choi et al. 2016)
Solar abundance set Anders & Grevesse (1989) solar abundance set
Nitrogen prescription Dopita et al. (2000) prescription
Depletion factor Depletion set described in Dopita et al. (2000)

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