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ESO 443-5

Observation

Spectrum ID98109150_sp1
Alt nameg1254248-282632
z0.0695
RA, Dec193.6034, -28.4421
MJD59019.48
SNR/Å B/R21.9/29.9
Obs Airmass1.16
SMSS ID98109150
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.4 ± 0.1
2MASS Kext11.6 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.053
Power law αν0.49 ± 0.01
log L5100,AGN44.19 ± 0.01
log HβBr/[O III]0.55 ± 0.01
log ML5100/M7.80 ± 0.03
log M/M7.61 ± 0.04
log M/M7.83 ± 0.03
log M[O III]/M7.75 ± 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 Narrow40.51 ± 0.35503 ± 63436 ± 290.71 ± 0.23
Hγ Broad42.04 ± 0.022530 ± 3211276 ± 3823.95 ± 0.44
[O III] 436440.27 ± 0.24396 ± 63167 ± 250.42 ± 0.13
He II Narrow40.12 ± 0.26396 ± 63167 ± 250.35 ± 0.14
He II Broad41.65 ± 0.0612742 ± 1475411 ± 6211.79 ± 0.88
Hβ Narrow41.30 ± 0.06503 ± 63437 ± 295.78 ± 0.29
Hβ Broad42.43 ± 0.012541 ± 881461 ± 3376.94 ± 0.59
[O III] 500741.87 ± 0.01503 ± 63437 ± 2923.33 ± 0.32
He I Narrow39.60 ± 0.39396 ± 63167 ± 250.18 ± 0.13
He I Broad41.71 ± 0.024343 ± 901844 ± 3723.63 ± 0.48
[O I] 630040.49 ± 0.06396 ± 63167 ± 251.71 ± 0.16
Hα Narrow41.63 ± 0.01396 ± 63167 ± 2526.05 ± 0.28
Hα Broad42.83 ± 0.011974 ± 641005 ± 25419.87 ± 0.72
[N II] 658541.26 ± 0.02396 ± 63167 ± 2511.26 ± 0.24
[S II] 671841.09 ± 0.02396 ± 63167 ± 258.00 ± 0.23
[S II] 673240.98 ± 0.02396 ± 63167 ± 256.23 ± 0.24

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 SNR59.35
Hβ Broad SNR22.78
Hγ Broad SNR11.64
AGN frac0.86
Host frac0.14
log L5100,Host43.41
Fe II/Hβ0.67
Fe II/[O III]2.36

Quality flags

spurious_hab/hbb0.0/0
l51002
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.