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2MASX J13541542-3746333

Observation

Spectrum ID99700135_sp1
Alt nameg1354154-374633
z0.0504
RA, Dec208.5642, -37.7759
MJD59732.46
SNR/Å B/R4.7/11.6
Obs Airmass1.01
SMSS ID99700135
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.6 ± 0.0
2MASS Kext11.5 ± 0.0

AGN Properties

Spectrum TypeSy 1.8
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.066
Power law αν-1.09 ± 0.65
log L5100,AGN42.99 ± 0.13
log HβBr/[O III]-1.39 ± 0.23
log ML5100/M6.96 ± 0.32
log M/M7.48 ± 0.13
log M/M6.93 ± 0.33
log M[O III]/M7.75 ± 0.31

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 Narrow40.99 ± 0.07338 ± 63187 ± 3243.17 ± 3.76
Hγ Broad40.91 ± 0.161212 ± 303578 ± 22233.91 ± 4.92
[O III] 436440.67 ± 0.09328 ± 63139 ± 2521.81 ± 2.28
He II Narrow40.75 ± 0.08328 ± 63139 ± 2528.20 ± 2.17
He II Broad40.64 ± 0.201388 ± 250589 ± 10620.38 ± 4.43
Hβ Narrow41.40 ± 0.02338 ± 63187 ± 32124.46 ± 3.48
Hβ Broad41.12 ± 0.231766 ± 617798 ± 88351.04 ± 5.74
[O III] 500742.51 ± 0.01338 ± 63187 ± 321696.15 ± 4.33
He I Narrow40.22 ± 0.15328 ± 63139 ± 2510.09 ± 1.36
He I Broad40.57 ± 0.213047 ± 15751294 ± 66924.53 ± 4.64
[O I] 630040.85 ± 0.03328 ± 63139 ± 2546.27 ± 1.50
Hα Narrow41.87 ± 0.02328 ± 63139 ± 25496.10 ± 2.39
Hα Broad42.09 ± 0.072893 ± 4211274 ± 413881.16 ± 6.19
[N II] 658541.65 ± 0.02328 ± 63139 ± 25298.13 ± 2.08
[S II] 671841.14 ± 0.02328 ± 63139 ± 2596.11 ± 1.80
[S II] 673241.18 ± 0.01328 ± 63139 ± 25105.72 ± 1.76

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 SNR8.54
Hβ Broad SNR1.76
Hγ Broad SNR1.66
AGN frac0.23
Host frac0.77
log L5100,Host43.51
Fe II/Hβ2.66
Fe II/[O III]0.08

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer1
balmer_snr2
hb_width0
balmer_width2

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.