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ESO 381-7

Observation

Spectrum ID97419092_sp1
Alt nameg1240470-333412
z0.0552
RA, Dec190.1957, -33.5699
MJD60081.43
SNR/Å B/R13.0/25.5
Obs Airmass1.02
SMSS ID97419092
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.8 ± 0.1
2MASS Kext11.7 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.068
Power law αν-0.96 ± 0.30
log L5100,AGN43.12 ± 0.05
log HβBr/[O III]-0.35 ± 0.02
log ML5100/M7.83 ± 0.08
log M/M7.70 ± 0.02
log M/M7.86 ± 0.08
log M[O III]/M8.17 ± 0.07

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 Narrow40.19 ± 0.16368 ± 63227 ± 265.06 ± 0.97
Hγ Broad40.63 ± 0.101883 ± 227655 ± 3413.80 ± 1.32
[O III] 436440.19 ± 0.08341 ± 63144 ± 255.12 ± 0.61
He II Narrow39.92 ± 0.16341 ± 63144 ± 252.95 ± 0.58
He II Broad39.83 ± 0.371694 ± 104719 ± 432.45 ± 1.26
Hβ Narrow40.69 ± 0.03368 ± 63227 ± 2618.17 ± 0.97
Hβ Broad41.39 ± 0.024470 ± 3801798 ± 4489.30 ± 2.42
[O III] 500741.74 ± 0.01368 ± 63227 ± 26206.25 ± 1.14
He I Narrow39.38 ± 0.37341 ± 63144 ± 251.06 ± 0.63
He I Broad40.08 ± 0.171180 ± 62501 ± 255.40 ± 1.11
[O I] 630040.53 ± 0.02341 ± 63144 ± 2516.20 ± 0.61
Hα Narrow41.17 ± 0.01341 ± 63144 ± 2573.46 ± 0.95
Hα Broad42.17 ± 0.013494 ± 761541 ± 25748.63 ± 2.98
[N II] 658541.24 ± 0.01341 ± 63144 ± 2586.95 ± 0.90
[S II] 671840.93 ± 0.01341 ± 63144 ± 2543.80 ± 0.74
[S II] 673240.84 ± 0.01341 ± 63144 ± 2535.90 ± 0.72

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 SNR20.56
Hβ Broad SNR3.91
Hγ Broad SNR1.98
AGN frac0.27
Host frac0.73
log L5100,Host43.55
Fe II/Hβ0.34
Fe II/[O III]0.15

Quality flags

spurious_hab/hbb0.0/0
l51001
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.