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ESO 543-11

Observation

Spectrum ID12403661_sp1
Alt nameg0140156-221445
z0.0865
RA, Dec25.0649, -22.2458
MJD60167.78
SNR/Å B/R18.0/23.8
Obs Airmass1.01
SMSS ID12403661
Closest SMSS6.15'', 2023359409
SMSS Mean r6"ap16.0 ± 0.0
2MASS Kext12.2 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.011
Power law αν0.14 ± 0.13
log L5100,AGN43.83 ± 0.02
log HβBr/[O III]0.12 ± 0.01
log ML5100/M8.13 ± 0.03
log M/M7.82 ± 0.04
log M/M8.23 ± 0.03
log M[O III]/M8.35 ± 0.03

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 Narrow40.71 ± 0.08440 ± 63309 ± 262.70 ± 0.29
Hγ Broad41.68 ± 0.023990 ± 3161574 ± 8725.73 ± 0.69
[O III] 436440.44 ± 0.09366 ± 63154 ± 251.46 ± 0.19
He II Narrow40.57 ± 0.06366 ± 63154 ± 252.32 ± 0.21
He II Broad41.71 ± 0.0310756 ± 5094568 ± 21632.00 ± 1.14
Hβ Narrow41.22 ± 0.02440 ± 63309 ± 2611.15 ± 0.35
Hβ Broad42.24 ± 0.014432 ± 1352490 ± 73118.34 ± 1.30
[O III] 500742.12 ± 0.01440 ± 63309 ± 2694.02 ± 0.42
He I Narrow40.21 ± 0.09366 ± 63154 ± 251.64 ± 0.26
He I Broad41.34 ± 0.034310 ± 2001830 ± 8522.27 ± 0.78
[O I] 630040.63 ± 0.03366 ± 63154 ± 255.00 ± 0.25
Hα Narrow41.51 ± 0.01366 ± 63154 ± 2541.90 ± 0.44
Hα Broad42.73 ± 0.012738 ± 671551 ± 25690.53 ± 1.37
[N II] 658541.37 ± 0.01366 ± 63154 ± 2530.48 ± 0.41
[S II] 671840.96 ± 0.02366 ± 63154 ± 2512.22 ± 0.34
[S II] 673240.89 ± 0.02366 ± 63154 ± 2510.62 ± 0.36

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 SNR49.33
Hβ Broad SNR13.23
Hγ Broad SNR5.63
AGN frac0.73
Host frac0.27
log L5100,Host43.39
Fe II/Hβ0.41
Fe II/[O III]0.55

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.