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2MASS J04352649-1643460

Observation

Spectrum ID22745338_sp1
Alt nameg0435265-164346
z0.0979
RA, Dec68.8604, -16.7295
MJD60581.72
SNR/Å B/R6.6/9.7
Obs Airmass1.05
SMSS ID22745338
Closest SMSSNone (< 15")
SMSS Mean r6"ap17.2 ± 0.2
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.062
Power law αν-0.99 ± 0.35
log L5100,AGN43.29 ± 0.04
log HβBr/[O III]0.52 ± 0.02
log ML5100/M7.43 ± 0.05
log M/M7.17 ± 0.03
log M/M7.56 ± 0.05
log M[O III]/M7.47 ± 0.05

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 Narrow39.79 ± 0.32270 ± 63183 ± 281.36 ± 0.82
Hγ Broad41.13 ± 0.052407 ± 189833 ± 6229.34 ± 1.89
[O III] 436439.95 ± 0.20239 ± 63100 ± 251.98 ± 0.61
He II Narrow40.10 ± 0.12239 ± 63100 ± 252.99 ± 0.55
He II Broad41.16 ± 0.089902 ± 2804205 ± 11934.10 ± 3.70
Hβ Narrow40.38 ± 0.11270 ± 63183 ± 286.00 ± 0.87
Hβ Broad41.79 ± 0.022589 ± 1331529 ± 74151.75 ± 3.34
[O III] 500741.27 ± 0.02270 ± 63183 ± 2847.33 ± 1.02
He I Narrow39.50 ± 0.27239 ± 63100 ± 250.93 ± 0.35
He I Broad40.71 ± 0.072930 ± 2061244 ± 8715.11 ± 1.42
[O I] 630039.29 ± 0.36239 ± 63100 ± 250.62 ± 0.42
Hα Narrow40.76 ± 0.03239 ± 63100 ± 2519.35 ± 0.56
Hα Broad42.17 ± 0.011902 ± 66913 ± 25491.30 ± 2.20
[N II] 658540.38 ± 0.06239 ± 63100 ± 258.04 ± 0.65
[S II] 671840.00 ± 0.08239 ± 63100 ± 253.44 ± 0.50
[S II] 673240.06 ± 0.08239 ± 63100 ± 253.91 ± 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 SNR25.47
Hβ Broad SNR9.43
Hγ Broad SNR3.28
AGN frac0.74
Host frac0.26
log L5100,Host42.84
Fe II/Hβ0.87
Fe II/[O III]2.88

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.