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2MASS J20473364-3613577

Observation

Spectrum ID233908272_sp1
Alt nameg2047337-361358
z0.0934
RA, Dec311.8902, -36.2326
MJD59823.46
SNR/Å B/R7.3/8.6
Obs Airmass1.04
SMSS ID233908272
Closest SMSS10.56'', 1273873386
SMSS Mean r6"ap16.2 ± 0.1
2MASS Kext12.7 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.044
Power law αν0.43 ± 0.07
log L5100,AGN43.40 ± 0.02
log HβBr/[O III]0.59 ± 0.10
log ML5100/M7.04 ± 0.10
log M/M6.58 ± 0.04
log M/M6.91 ± 0.11
log M[O III]/M6.76 ± 0.11

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 Narrow40.18 ± 0.25321 ± 66492 ± 352.08 ± 0.86
Hγ Broad40.68 ± 0.142060 ± 320718 ± 735.90 ± 1.17
[O III] 436439.56 ± 0.39257 ± 63108 ± 250.50 ± 0.37
He II Narrow39.42 ± 0.43257 ± 63108 ± 250.43 ± 0.38
He II Broad39.74 ± 0.451225 ± 65520 ± 260.89 ± 0.85
Hβ Narrow40.99 ± 0.07321 ± 66492 ± 3517.30 ± 1.05
Hβ Broad41.29 ± 0.071580 ± 1782680 ± 12135.10 ± 2.89
[O III] 500740.70 ± 0.07321 ± 66492 ± 359.59 ± 1.20
He I Narrow39.62 ± 0.22257 ± 63108 ± 251.19 ± 0.33
He I Broad40.34 ± 0.122035 ± 68864 ± 286.22 ± 0.97
[O I] 630039.92 ± 0.11257 ± 63108 ± 252.82 ± 0.43
Hα Narrow40.95 ± 0.02257 ± 63108 ± 2533.21 ± 0.49
Hα Broad41.65 ± 0.011390 ± 65601 ± 25166.20 ± 1.50
[N II] 658540.61 ± 0.02257 ± 63108 ± 2515.57 ± 0.48
[S II] 671840.02 ± 0.08257 ± 63108 ± 254.20 ± 0.56
[S II] 673240.13 ± 0.07257 ± 63108 ± 255.35 ± 0.53

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 SNR11.36
Hβ Broad SNR2.88
Hγ Broad SNR1.39
AGN frac0.82
Host frac0.18
log L5100,Host42.75
Fe II/Hβ1.57
Fe II/[O III]6.18

Quality flags

spurious_hab/hbb0.0/0
l51002
balmer1
balmer_snr1
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.