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2MASS J13283109-4909060

Observation

Spectrum ID320346080_sp1
Alt nameg1328311-490906
z0.0476
RA, Dec202.1295, -49.1517
MJD60058.44
SNR/Å B/R16.9/20.7
Obs Airmass1.25
SMSS ID320346080
Closest SMSS6.92'', 320346078
SMSS Mean r6"ap16.4 ± 0.1
2MASS Kext12.6 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.129
Power law αν0.35 ± 0.11
log L5100,AGN43.18 ± 0.02
log HβBr/[O III]0.29 ± 0.01
log ML5100/M7.74 ± 0.03
log M/M7.45 ± 0.02
log M/M7.84 ± 0.04
log M[O III]/M7.85 ± 0.03

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 Narrow39.83 ± 0.12274 ± 63146 ± 251.56 ± 0.31
Hγ Broad41.01 ± 0.033915 ± 2701487 ± 7023.36 ± 0.94
[O III] 436439.44 ± 0.22250 ± 63105 ± 250.64 ± 0.21
He II Narrow39.86 ± 0.08250 ± 63105 ± 252.00 ± 0.22
He II Broad41.00 ± 0.035558 ± 2082360 ± 8827.76 ± 1.27
Hβ Narrow40.37 ± 0.03274 ± 63146 ± 257.06 ± 0.33
Hβ Broad41.58 ± 0.013954 ± 1243335 ± 87116.44 ± 2.01
[O III] 500741.29 ± 0.01274 ± 63146 ± 2563.80 ± 0.37
He I Narrow39.19 ± 0.25250 ± 63105 ± 250.73 ± 0.27
He I Broad40.67 ± 0.043928 ± 1781668 ± 7521.98 ± 1.25
[O I] 630039.87 ± 0.05250 ± 63105 ± 254.16 ± 0.34
Hα Narrow40.87 ± 0.01250 ± 63105 ± 2544.95 ± 0.57
Hα Broad41.93 ± 0.013116 ± 681633 ± 31524.23 ± 2.44
[N II] 658540.66 ± 0.01250 ± 63105 ± 2527.92 ± 0.50
[S II] 671840.19 ± 0.03250 ± 63105 ± 2510.01 ± 0.41
[S II] 673240.20 ± 0.03250 ± 63105 ± 2510.26 ± 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 SNR22.32
Hβ Broad SNR8.37
Hγ Broad SNR3.92
AGN frac0.51
Host frac0.49
log L5100,Host43.16
Fe II/Hβ0.30
Fe II/[O III]0.57

Quality flags

spurious_hab/hbb0.0/0
l51002
balmer0
balmer_snr0
hb_width2
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.