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MCG-02-12-045

Observation

Spectrum ID24393139_sp1
Alt nameg0436223-102234
z0.0353
RA, Dec69.0929, -10.3760
MJD60566.77
SNR/Å B/R9.3/14.6
Obs Airmass1.08
SMSS ID24393139
Closest SMSSNone (< 15")
SMSS Mean r6"ap14.8 ± 0.2
2MASS Kext10.4 ± 0.0

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.065
Power law αν0.13 ± 0.15
log L5100,AGN43.55 ± 0.02
log HβBr/[O III]0.25 ± 0.02
log ML5100/M7.69 ± 0.05
log M/M7.32 ± 0.05
log M/M7.71 ± 0.05
log M[O III]/M7.75 ± 0.05

Spatial extraction & sky subtraction region

Spatial plot

Spaxel scale: 1 arcsec² — Flux units: erg s⁻¹ cm⁻² Å⁻¹
Apertures: object (solid), background (dashed)

Spectrum decomposition

Emission line measurements

Linelog L (erg s⁻¹)FWHM (km s⁻¹)σ (km s⁻¹)EW (Å)
Hγ Narrow40.35 ± 0.19790 ± 67268 ± 262.37 ± 0.40
Hγ Broad41.27 ± 0.052438 ± 224928 ± 8919.17 ± 0.91
[O III] 436440.12 ± 0.19399 ± 72169 ± 291.45 ± 0.35
He II Narrow39.77 ± 0.34399 ± 72169 ± 290.76 ± 0.33
He II Broad40.72 ± 0.101303 ± 115553 ± 486.13 ± 0.60
Hβ Narrow40.82 ± 0.07790 ± 67268 ± 268.67 ± 0.38
Hβ Broad41.78 ± 0.023091 ± 1761109 ± 10774.81 ± 1.01
[O III] 500741.53 ± 0.01790 ± 67268 ± 2646.63 ± 0.47
He I Narrow39.33 ± 0.37399 ± 72169 ± 290.44 ± 0.28
He I Broad40.95 ± 0.092470 ± 4931049 ± 20916.89 ± 0.72
[O I] 630039.96 ± 0.12399 ± 72169 ± 292.16 ± 0.33
Hα Narrow41.14 ± 0.04399 ± 72169 ± 2934.47 ± 0.66
Hα Broad42.27 ± 0.012106 ± 121973 ± 68462.06 ± 1.38
[N II] 658541.05 ± 0.08399 ± 72169 ± 2927.53 ± 0.63
[S II] 671840.43 ± 0.06399 ± 72169 ± 297.29 ± 0.43
[S II] 673240.43 ± 0.05399 ± 72169 ± 297.21 ± 0.41

All narrow line widths are tied to narrow [O III] 5007Å. [O III] 5007Å and narrow Hβ include a second narrow component not tied to other narrow lines.

Emission summary

Hα Broad SNR31.20
Hβ Broad SNR10.14
Hγ Broad SNR4.53
AGN frac0.84
Host frac0.16
log L5100,Host42.83
Fe II/Hβ0.53
Fe II/[O III]0.91

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width0
balmer_width0

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.