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ESO 140-43

Observation

Spectrum ID478399456_sp1
Alt nameg1844540-622153
z0.0139
RA, Dec281.2249, -62.3647
MJD59492.38
SNR/Å B/R8.8/19.6
Obs Airmass1.20
SMSS ID478399456
Closest SMSSNone (< 15")
SMSS Mean r6"ap14.4 ± 0.1
2MASS Kext9.7 ± 0.0

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.093
Power law αν-1.77 ± 0.18
log L5100,AGN43.10 ± 0.02
log HβBr/[O III]-0.01 ± 0.04
log ML5100/M7.55 ± 0.06
log M/M7.11 ± 0.09
log M/M7.53 ± 0.06
log M[O III]/M7.68 ± 0.06

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 Narrow39.75 ± 0.20284 ± 63210 ± 432.16 ± 0.68
Hγ Broad40.52 ± 0.081655 ± 330538 ± 10612.43 ± 1.04
[O III] 436439.69 ± 0.16260 ± 63109 ± 251.93 ± 0.40
He II Narrow39.53 ± 0.20260 ± 63109 ± 251.36 ± 0.30
He II Broad40.45 ± 0.172277 ± 781967 ± 33111.16 ± 0.91
Hβ Narrow40.29 ± 0.04284 ± 63210 ± 437.63 ± 0.53
Hβ Broad41.25 ± 0.043305 ± 1991424 ± 23175.96 ± 1.35
[O III] 500741.26 ± 0.01284 ± 63210 ± 4373.62 ± 0.55
He I Narrow39.04 ± 0.31260 ± 63109 ± 250.46 ± 0.16
He I Broad40.30 ± 0.181713 ± 795727 ± 3378.20 ± 0.44
[O I] 630039.62 ± 0.07260 ± 63109 ± 251.82 ± 0.17
Hα Narrow40.79 ± 0.02260 ± 63109 ± 2526.30 ± 0.28
Hα Broad41.88 ± 0.012169 ± 2431038 ± 67324.65 ± 0.76
[N II] 658540.67 ± 0.04260 ± 63109 ± 2520.06 ± 0.24
[S II] 671840.21 ± 0.02260 ± 63109 ± 257.03 ± 0.18
[S II] 673240.19 ± 0.03260 ± 63109 ± 256.71 ± 0.19

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 SNR33.90
Hβ Broad SNR7.60
Hγ Broad SNR3.29
AGN frac0.81
Host frac0.18
log L5100,Host42.45
Fe II/Hβ0.50
Fe II/[O III]0.52

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.