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ESO 264-52

Observation

Spectrum ID410366359_sp1
Alt nameg1057139-474011
z0.0154
RA, Dec164.3079, -47.6698
MJD60413.43
SNR/Å B/R13.5/19.1
Obs Airmass1.07
SMSS ID410366359
Closest SMSS11.17'', 410366146
SMSS Mean r6"ap15.6 ± 0.1
2MASS Kext11.3 ± 0.1

AGN Properties

Spectrum TypeSy 1.8
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.165
Power law αν-1.06 ± 0.11
log L5100,AGN42.45 ± 0.02
log HβBr/[O III]-0.78 ± 0.07
log ML5100/M7.13 ± 0.23
log M/M6.57 ± 0.06
log M/M6.99 ± 0.24
log M[O III]/M7.48 ± 0.23

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 Narrow39.86 ± 0.05279 ± 62209 ± 2811.11 ± 0.70
Hγ Broad39.77 ± 0.131409 ± 205513 ± 817.97 ± 0.90
[O III] 436439.38 ± 0.07264 ± 63110 ± 253.75 ± 0.37
He II Narrow39.14 ± 0.12264 ± 63110 ± 252.32 ± 0.31
He II Broad39.95 ± 0.112038 ± 348866 ± 14813.78 ± 0.88
Hβ Narrow40.31 ± 0.02279 ± 62209 ± 2834.77 ± 0.61
Hβ Broad40.39 ± 0.072781 ± 650991 ± 20640.79 ± 1.07
[O III] 500741.17 ± 0.01279 ± 62210 ± 28259.90 ± 0.74
He I Narrow39.07 ± 0.12264 ± 63110 ± 252.40 ± 0.29
He I Broad39.56 ± 0.091488 ± 206632 ± 877.79 ± 0.71
[O I] 630039.77 ± 0.02264 ± 63110 ± 2512.84 ± 0.31
Hα Narrow40.74 ± 0.01264 ± 63110 ± 25127.07 ± 0.48
Hα Broad41.10 ± 0.012029 ± 119841 ± 62298.63 ± 1.14
[N II] 658540.27 ± 0.02264 ± 63110 ± 2542.64 ± 0.38
[S II] 671840.02 ± 0.01264 ± 63110 ± 2524.68 ± 0.36
[S II] 673239.99 ± 0.01264 ± 63110 ± 2523.04 ± 0.38

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 SNR24.78
Hβ Broad SNR5.03
Hγ Broad SNR2.38
AGN frac0.46
Host frac0.54
log L5100,Host42.52
Fe II/Hβ0.55
Fe II/[O III]0.09

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.