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ESO 438-9

Observation

Spectrum ID87235021_sp1
Alt nameg1110480-283004
z0.0238
RA, Dec167.7000, -28.5010
MJD60382.41
SNR/Å B/R24.1/32.6
Obs Airmass1.59
SMSS ID87235021
Closest SMSS13.18'', 87235022
SMSS Mean r6"ap14.7 ± 0.1
2MASS Kext10.6 ± 0.0

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.054
Power law αν-0.87 ± 0.06
log L5100,AGN43.25 ± 0.01
log HβBr/[O III]0.08 ± 0.02
log ML5100/M7.25 ± 0.06
log M/M6.76 ± 0.04
log M/M7.04 ± 0.07
log M[O III]/M7.13 ± 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 Narrow40.16 ± 0.04314 ± 63232 ± 263.41 ± 0.21
Hγ Broad40.25 ± 0.082310 ± 173779 ± 384.04 ± 0.36
[O III] 436439.33 ± 0.17260 ± 62109 ± 250.51 ± 0.12
He II Narrow39.25 ± 0.16260 ± 62109 ± 250.46 ± 0.11
He II Broad39.22 ± 0.434113 ± 2021747 ± 850.43 ± 0.39
Hβ Narrow40.63 ± 0.01314 ± 63232 ± 2611.47 ± 0.19
Hβ Broad40.96 ± 0.012167 ± 132978 ± 3324.78 ± 0.38
[O III] 500740.88 ± 0.01314 ± 63232 ± 2621.14 ± 0.19
He I Narrow39.46 ± 0.08260 ± 62109 ± 250.97 ± 0.10
He I Broad40.48 ± 0.033390 ± 1081439 ± 4510.10 ± 0.39
[O I] 630039.67 ± 0.04260 ± 62109 ± 251.70 ± 0.11
Hα Narrow41.08 ± 0.01260 ± 62109 ± 2545.11 ± 0.17
Hα Broad41.60 ± 0.011785 ± 65722 ± 25149.22 ± 0.41
[N II] 658540.92 ± 0.01260 ± 62109 ± 2531.44 ± 0.16
[S II] 671840.28 ± 0.01260 ± 62109 ± 257.45 ± 0.15
[S II] 673240.24 ± 0.01260 ± 62109 ± 256.76 ± 0.13

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 SNR39.84
Hβ Broad SNR10.12
Hγ Broad SNR2.28
AGN frac0.78
Host frac0.22
log L5100,Host42.71
Fe II/Hβ1.72
Fe II/[O III]2.09

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
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.