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2MASS J08545518-2423373

Observation

Spectrum ID47283434_sp1
Alt nameg0854552-242338
z0.0911
RA, Dec133.7300, -24.3937
MJD60057.37
SNR/Å B/R23.5/24.7
Obs Airmass1.01
SMSS ID47283434
Closest SMSS14.10'', 1056835739
SMSS Mean r6"apnan ± nan
2MASS Kext12.3 ± 0.1

AGN Properties

Spectrum TypeSy 1.0
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.137
Power law αν0.49 ± 0.01
log L5100,AGN43.86 ± 0.01
log HβBr/[O III]0.86 ± 0.02
log ML5100/M8.28 ± 0.01
log M/M8.08 ± 0.03
log M/M8.38 ± 0.01
log M[O III]/M8.13 ± 0.02

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 Narrow39.84 ± 0.42724 ± 66509 ± 280.32 ± 0.24
Hγ Broad41.63 ± 0.023721 ± 2311451 ± 2719.99 ± 0.46
[O III] 436440.03 ± 0.28621 ± 63263 ± 250.51 ± 0.18
He II Narrow39.64 ± 0.44621 ± 63263 ± 250.25 ± 0.18
He II Broad40.61 ± 0.122185 ± 65928 ± 262.32 ± 0.34
Hβ Narrow40.71 ± 0.08724 ± 66510 ± 283.18 ± 0.32
Hβ Broad42.24 ± 0.015215 ± 822057 ± 25108.68 ± 0.67
[O III] 500741.38 ± 0.02724 ± 66510 ± 2816.03 ± 0.35
He I Narrow40.09 ± 0.16621 ± 63263 ± 251.24 ± 0.24
He I Broad41.26 ± 0.034857 ± 652063 ± 2618.08 ± 0.79
[O I] 630040.02 ± 0.19621 ± 63263 ± 251.23 ± 0.34
Hα Narrow41.24 ± 0.02621 ± 63263 ± 2522.65 ± 0.45
Hα Broad42.63 ± 0.013931 ± 691609 ± 25555.63 ± 1.19
[N II] 658540.16 ± 0.23621 ± 63263 ± 251.92 ± 0.42
[S II] 671840.32 ± 0.11621 ± 63263 ± 252.95 ± 0.47
[S II] 673240.55 ± 0.06621 ± 63263 ± 254.94 ± 0.50

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 SNR41.44
Hβ Broad SNR17.82
Hγ Broad SNR7.19
AGN frac0.78
Host frac0.22
log L5100,Host43.30
Fe II/Hβ0.69
Fe II/[O III]4.99

Quality flags

spurious_hab/hbb0.0/0
l51002
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.