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2MASS J05542641-3453402

Observation

Spectrum ID19969626_sp1
Alt nameg0554264-345341
z0.0817
RA, Dec88.6100, -34.8946
MJD60341.46
SNR/Å B/R17.0/17.6
Obs Airmass1.00
SMSS ID19969626
Closest SMSS13.04'', 2041780666
SMSS Mean r6"ap16.5 ± 0.0
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.035
Power law αν0.14 ± 0.08
log L5100,AGN43.81 ± 0.01
log HβBr/[O III]0.52 ± 0.01
log ML5100/M7.32 ± 0.03
log M/M7.06 ± 0.04
log M/M7.36 ± 0.03
log M[O III]/M7.28 ± 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 Narrow40.26 ± 0.21315 ± 63344 ± 351.00 ± 0.30
Hγ Broad41.63 ± 0.021709 ± 132717 ± 3823.63 ± 0.45
[O III] 436439.89 ± 0.24299 ± 63126 ± 250.44 ± 0.15
He II Narrow40.26 ± 0.09299 ± 63126 ± 251.18 ± 0.18
He II Broad41.59 ± 0.038903 ± 3333781 ± 14125.36 ± 0.92
Hβ Narrow41.01 ± 0.04315 ± 63344 ± 357.23 ± 0.37
Hβ Broad42.08 ± 0.011762 ± 551002 ± 4285.92 ± 0.74
[O III] 500741.57 ± 0.01315 ± 63344 ± 3527.82 ± 0.40
He I Narrow39.94 ± 0.16299 ± 63126 ± 250.92 ± 0.22
He I Broad41.11 ± 0.043189 ± 1831354 ± 7713.64 ± 0.69
[O I] 630040.04 ± 0.10299 ± 63126 ± 251.36 ± 0.22
Hα Narrow41.34 ± 0.02299 ± 63126 ± 2529.55 ± 0.40
Hα Broad42.48 ± 0.011351 ± 63709 ± 25400.28 ± 1.15
[N II] 658540.98 ± 0.02299 ± 63126 ± 2512.84 ± 0.33
[S II] 671840.67 ± 0.03299 ± 63126 ± 256.58 ± 0.42
[S II] 673240.54 ± 0.05299 ± 63126 ± 254.88 ± 0.44

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 SNR64.89
Hβ Broad SNR25.98
Hγ Broad SNR12.39
AGN frac0.84
Host frac0.16
log L5100,Host43.10
Fe II/Hβ0.68
Fe II/[O III]2.24

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
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.