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MCG-02-35-001

Observation

Spectrum ID107402694_sp1
Alt nameg1332391-102853
z0.0223
RA, Dec203.1630, -10.4813
MJD59015.52
SNR/Å B/R19.3/37.9
Obs Airmass1.31
SMSS ID107402694
Closest SMSS3.58'', 2174311836
SMSS Mean r6"ap15.6 ± 0.1
2MASS Kext11.3 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.045
Power law αν-0.72 ± 0.08
log L5100,AGN42.81 ± 0.01
log HβBr/[O III]0.49 ± 0.02
log ML5100/M6.97 ± 0.04
log M/M6.38 ± 0.05
log M/M6.86 ± 0.05
log M[O III]/M6.75 ± 0.06

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 Narrow39.12 ± 0.22265 ± 63167 ± 270.84 ± 0.27
Hγ Broad40.36 ± 0.032102 ± 236836 ± 5614.65 ± 0.62
[O III] 436439.08 ± 0.16226 ± 6394 ± 250.77 ± 0.17
He II Narrow39.00 ± 0.14226 ± 6394 ± 250.70 ± 0.15
He II Broad39.42 ± 0.213161 ± 2611342 ± 1101.91 ± 0.57
Hβ Narrow39.78 ± 0.04265 ± 63167 ± 274.39 ± 0.25
Hβ Broad40.79 ± 0.011941 ± 65920 ± 4145.62 ± 0.70
[O III] 500740.30 ± 0.01265 ± 63167 ± 2715.30 ± 0.25
He I Narrow38.71 ± 0.16226 ± 6394 ± 250.48 ± 0.11
He I Broad40.22 ± 0.033983 ± 1951691 ± 8215.59 ± 0.50
[O I] 630038.80 ± 0.11226 ± 6394 ± 250.65 ± 0.12
Hα Narrow40.11 ± 0.01226 ± 6394 ± 2514.02 ± 0.18
Hα Broad41.34 ± 0.011373 ± 63662 ± 25236.19 ± 0.55
[N II] 658539.95 ± 0.01226 ± 6394 ± 259.73 ± 0.15
[S II] 671839.35 ± 0.05226 ± 6394 ± 252.50 ± 0.17
[S II] 673239.31 ± 0.04226 ± 6394 ± 252.28 ± 0.15

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 SNR48.79
Hβ Broad SNR13.40
Hγ Broad SNR5.82
AGN frac0.62
Host frac0.38
log L5100,Host42.60
Fe II/Hβ1.06
Fe II/[O III]3.27

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.