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MCG-04-32-029

Observation

Spectrum ID99381978_sp1
Alt nameg1331138-252410
z0.0266
RA, Dec202.8077, -25.4027
MJD61067.74
SNR/Å B/R16.7/35.4
Obs Airmass1.07
SMSS ID99381978
Closest SMSSNone (< 15")
SMSS Mean r6"ap14.7 ± 0.1
2MASS Kext10.8 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.059
Power law αν-1.16 ± 0.35
log L5100,AGN42.82 ± 0.04
log HβBr/[O III]-0.02 ± 0.02
log ML5100/M7.90 ± 0.07
log M/M7.63 ± 0.02
log M/M7.99 ± 0.08
log M[O III]/M8.14 ± 0.07

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 Narrow39.63 ± 0.26681 ± 63278 ± 252.90 ± 0.74
Hγ Broad40.23 ± 0.102036 ± 197668 ± 3310.95 ± 1.32
[O III] 436439.91 ± 0.09569 ± 63241 ± 255.52 ± 0.72
He II Narrow39.51 ± 0.23569 ± 63241 ± 252.32 ± 0.56
He II Broad39.33 ± 0.411214 ± 64515 ± 261.52 ± 0.81
Hβ Narrow40.20 ± 0.05681 ± 63278 ± 2511.86 ± 0.67
Hβ Broad41.22 ± 0.025653 ± 4383073 ± 61124.34 ± 2.49
[O III] 500741.24 ± 0.01681 ± 63279 ± 25133.45 ± 0.72
He I Narrow39.30 ± 0.27569 ± 63241 ± 251.74 ± 0.38
He I Broad39.51 ± 0.241179 ± 62500 ± 252.81 ± 0.55
[O I] 630040.14 ± 0.03569 ± 63241 ± 2512.71 ± 0.45
Hα Narrow40.77 ± 0.01569 ± 63241 ± 2556.01 ± 0.63
Hα Broad41.73 ± 0.014403 ± 871831 ± 25509.78 ± 1.62
[N II] 658540.93 ± 0.01569 ± 63241 ± 2581.71 ± 0.61
[S II] 671840.49 ± 0.01569 ± 63241 ± 2529.85 ± 0.56
[S II] 673240.44 ± 0.01569 ± 63241 ± 2527.13 ± 0.56

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 SNR18.19
Hβ Broad SNR5.09
Hγ Broad SNR2.12
AGN frac0.32
Host frac0.68
log L5100,Host43.16
Fe II/Hβ0.63
Fe II/[O III]0.60

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr1
hb_width1
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.