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ESO 209-12

Observation

Spectrum ID467114720_sp1
Alt nameg0801580-494642
z0.0404
RA, Dec120.4915, -49.7784
MJD60286.69
SNR/Å B/R13.6/25.4
Obs Airmass1.06
SMSS ID467114720
Closest SMSS7.85'', 2666234809
SMSS Mean r6"ap15.2 ± 0.1
2MASS Kext10.1 ± 0.0

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.225
Power law αν-0.37 ± 0.26
log L5100,AGN43.61 ± 0.05
log HβBr/[O III]-0.33 ± 0.11
log ML5100/M8.00 ± 0.29
log M/M8.10 ± 0.04
log M/M7.98 ± 0.30
log M[O III]/M8.31 ± 0.29

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 Narrow40.75 ± 0.12606 ± 63261 ± 265.20 ± 0.51
Hγ Broad40.93 ± 0.241929 ± 596775 ± 4167.04 ± 0.95
[O III] 436440.63 ± 0.12601 ± 63255 ± 254.19 ± 0.48
He II Narrow40.52 ± 0.13601 ± 63255 ± 253.63 ± 0.47
He II Broad40.77 ± 0.281764 ± 1701749 ± 7223.92 ± 0.76
Hβ Narrow41.09 ± 0.08606 ± 63261 ± 2614.26 ± 0.50
Hβ Broad41.74 ± 0.114305 ± 14731614 ± 58663.32 ± 1.27
[O III] 500742.07 ± 0.01606 ± 63261 ± 26143.55 ± 0.59
He I Narrow40.27 ± 0.15601 ± 63255 ± 252.93 ± 0.36
He I Broad40.72 ± 0.281701 ± 1110722 ± 4717.46 ± 0.60
[O I] 630040.65 ± 0.04601 ± 63255 ± 257.84 ± 0.49
Hα Narrow41.69 ± 0.02601 ± 63255 ± 2593.52 ± 0.72
Hα Broad42.41 ± 0.014690 ± 1931739 ± 96474.01 ± 1.50
[N II] 658541.75 ± 0.02601 ± 63255 ± 25107.30 ± 0.74
[S II] 671841.27 ± 0.02601 ± 63255 ± 2536.39 ± 0.53
[S II] 673241.21 ± 0.02601 ± 63255 ± 2531.84 ± 0.51

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 SNR17.15
Hβ Broad SNR5.46
Hγ Broad SNR1.91
AGN frac0.52
Host frac0.47
log L5100,Host43.57
Fe II/Hβ1.10
Fe II/[O III]0.51

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
hb_width0
balmer_width1

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