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2MASS J13543948-4214564

Observation

Spectrum ID308129573_sp1
Alt nameg1354395-421457
z0.0763
RA, Dec208.6645, -42.2490
MJD60382.77
SNR/Å B/R17.4/16.8
Obs Airmass1.10
SMSS ID308129573
Closest SMSS12.95'', 1373820705
SMSS Mean r6"ap15.7 ± 0.1
2MASS Kext11.9 ± 0.0

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.070
Power law αν0.42 ± 0.06
log L5100,AGN43.92 ± 0.01
log HβBr/[O III]0.42 ± 0.01
log ML5100/M7.59 ± 0.02
log M/M7.46 ± 0.04
log M/M7.67 ± 0.02
log M[O III]/M7.65 ± 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 Narrow40.60 ± 0.09264 ± 63176 ± 251.64 ± 0.18
Hγ Broad41.82 ± 0.022186 ± 1801077 ± 4727.39 ± 0.52
[O III] 436440.12 ± 0.16247 ± 63104 ± 250.56 ± 0.13
He II Narrow40.31 ± 0.09247 ± 63104 ± 251.02 ± 0.14
He II Broad41.61 ± 0.035296 ± 2222249 ± 9420.15 ± 0.65
Hβ Narrow40.93 ± 0.04264 ± 63176 ± 254.62 ± 0.23
Hβ Broad42.27 ± 0.012287 ± 471372 ± 44101.65 ± 0.88
[O III] 500741.86 ± 0.01264 ± 63176 ± 2541.62 ± 0.28
He I Narrow39.65 ± 0.27247 ± 63104 ± 250.38 ± 0.17
He I Broad41.43 ± 0.022617 ± 1181111 ± 4922.74 ± 0.61
[O I] 630040.27 ± 0.07247 ± 63104 ± 251.89 ± 0.19
Hα Narrow41.47 ± 0.01247 ± 63104 ± 2532.91 ± 0.36
Hα Broad42.64 ± 0.011904 ± 65938 ± 25490.50 ± 1.13
[N II] 658540.90 ± 0.02247 ± 63104 ± 258.88 ± 0.29
[S II] 671840.80 ± 0.02247 ± 63104 ± 257.39 ± 0.30
[S II] 673240.67 ± 0.04247 ± 63104 ± 255.53 ± 0.35

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 SNR56.75
Hβ Broad SNR24.73
Hγ Broad SNR11.31
AGN frac0.87
Host frac0.13
log L5100,Host43.11
Fe II/Hβ0.51
Fe II/[O III]1.34

Quality flags

spurious_hab/hbb0.0/0
l51002
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.