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EC 14040-2428

Observation

Spectrum ID102488645_sp1
Alt nameg1406507-244250
z0.0454
RA, Dec211.7114, -24.7138
MJD59019.5
SNR/Å B/R22.1/37.3
Obs Airmass1.08
SMSS ID102488645
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.1 ± 0.1
2MASS Kext12.4 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.058
Power law αν0.15 ± 0.13
log L5100,AGN43.38 ± 0.02
log HβBr/[O III]0.13 ± 0.01
log ML5100/M7.37 ± 0.05
log M/M6.75 ± 0.04
log M/M7.26 ± 0.05
log M[O III]/M7.34 ± 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 Narrow40.28 ± 0.06309 ± 63248 ± 272.86 ± 0.25
Hγ Broad40.50 ± 0.061236 ± 75403 ± 254.56 ± 0.30
[O III] 436439.99 ± 0.06281 ± 62117 ± 251.49 ± 0.14
He II Narrow39.77 ± 0.09281 ± 62117 ± 251.06 ± 0.13
He II Broad40.57 ± 0.052692 ± 1181143 ± 496.54 ± 0.43
Hβ Narrow40.78 ± 0.02309 ± 63248 ± 2711.52 ± 0.27
Hβ Broad41.31 ± 0.012336 ± 1171001 ± 3039.01 ± 0.48
[O III] 500741.18 ± 0.01309 ± 63248 ± 2730.87 ± 0.28
He I Narrow39.55 ± 0.09281 ± 62117 ± 251.03 ± 0.12
He I Broad40.57 ± 0.032488 ± 921057 ± 3810.68 ± 0.37
[O I] 630039.76 ± 0.04281 ± 62117 ± 251.94 ± 0.14
Hα Narrow41.22 ± 0.01281 ± 62117 ± 2561.37 ± 0.25
Hα Broad41.81 ± 0.011517 ± 63732 ± 25236.28 ± 0.57
[N II] 658540.96 ± 0.01281 ± 62117 ± 2533.78 ± 0.22
[S II] 671840.46 ± 0.01281 ± 62117 ± 2511.07 ± 0.17
[S II] 673240.35 ± 0.01281 ± 62117 ± 258.79 ± 0.17

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 SNR43.82
Hβ Broad SNR13.34
Hγ Broad SNR4.58
AGN frac0.69
Host frac0.31
log L5100,Host43.04
Fe II/Hβ1.42
Fe II/[O III]1.91

Quality flags

spurious_hab/hbb0.0/0
l51000
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.