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2MASX J08432682-0951207

Observation

Spectrum ID75378764_sp1
Alt nameg0843268-095121
z0.0410
RA, Dec130.8616, -9.8557
MJD60021.45
SNR/Å B/R10.2/23.0
Obs Airmass1.08
SMSS ID75378764
Closest SMSS4.61'', 2113897105
SMSS Mean r6"ap16.9 ± 0.1
2MASS Kext13.2 ± 0.2

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.038
Power law αν-0.66 ± 0.24
log L5100,AGN42.69 ± 0.04
log HβBr/[O III]0.18 ± 0.03
log ML5100/M7.34 ± 0.10
log M/M6.68 ± 0.04
log M/M7.29 ± 0.10
log M[O III]/M7.33 ± 0.10

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 Narrow39.49 ± 0.16212 ± 63270 ± 302.58 ± 0.99
Hγ Broad40.19 ± 0.092095 ± 125774 ± 4312.25 ± 1.43
[O III] 436439.15 ± 0.24203 ± 6385 ± 251.17 ± 0.41
He II Narrow38.73 ± 0.40203 ± 6385 ± 250.50 ± 0.37
He II Broad40.68 ± 0.0612950 ± 625499 ± 2544.05 ± 3.22
Hβ Narrow39.78 ± 0.07212 ± 63270 ± 305.86 ± 0.91
Hβ Broad40.81 ± 0.023157 ± 3311362 ± 4061.66 ± 1.78
[O III] 500740.62 ± 0.02212 ± 63270 ± 3042.44 ± 0.98
He I Narrow38.79 ± 0.21203 ± 6385 ± 250.77 ± 0.23
He I Broad40.24 ± 0.043659 ± 791554 ± 3221.77 ± 1.05
[O I] 630039.07 ± 0.11203 ± 6385 ± 251.59 ± 0.26
Hα Narrow40.18 ± 0.01203 ± 6385 ± 2521.94 ± 0.33
Hα Broad41.27 ± 0.012047 ± 751046 ± 25271.77 ± 1.27
[N II] 658540.15 ± 0.01203 ± 6385 ± 2520.62 ± 0.32
[S II] 671839.70 ± 0.03203 ± 6385 ± 257.40 ± 0.30
[S II] 673239.58 ± 0.04203 ± 6385 ± 255.67 ± 0.29

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 SNR14.55
Hβ Broad SNR4.88
Hγ Broad SNR2.10
AGN frac0.46
Host frac0.54
log L5100,Host42.77
Fe II/Hβ0.56
Fe II/[O III]0.85

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr1
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.