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ESO 327-25

Observation

Spectrum ID308543986_sp3
Alt nameg1452310-422625
z0.0498
RA, Dec223.1292, -42.4402
MJD59725.51
SNR/Å B/R17.3/40.9
Obs Airmass1.03
SMSS ID308543986
Closest SMSS9.99'', 308543989
SMSS Mean r6"ap15.6 ± 0.0
2MASS Kext10.9 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.101
Power law αν-1.37 ± 0.19
log L5100,AGN43.47 ± 0.04
log HβBr/[O III]0.37 ± 0.03
log ML5100/M7.50 ± 0.25
log M/M7.26 ± 0.03
log M/M7.46 ± 0.25
log M[O III]/M7.43 ± 0.25

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 Narrow40.02 ± 0.29535 ± 63256 ± 361.63 ± 0.83
Hγ Broad40.47 ± 0.161227 ± 66431 ± 253.95 ± 0.89
[O III] 436439.60 ± 0.43526 ± 63223 ± 250.63 ± 0.57
He II Narrow39.51 ± 0.48526 ± 63223 ± 250.53 ± 0.48
He II Broad39.91 ± 0.391479 ± 64628 ± 251.32 ± 0.82
Hβ Narrow40.52 ± 0.14535 ± 63257 ± 365.48 ± 0.74
Hβ Broad41.57 ± 0.022588 ± 6911847 ± 5562.19 ± 1.69
[O III] 500741.20 ± 0.02535 ± 63257 ± 3626.67 ± 0.78
He I Narrow40.09 ± 0.10526 ± 63223 ± 252.34 ± 0.31
He I Broad40.87 ± 0.075785 ± 642456 ± 2614.06 ± 1.03
[O I] 630039.44 ± 0.34526 ± 63223 ± 250.54 ± 0.30
Hα Narrow41.17 ± 0.02526 ± 63223 ± 2530.14 ± 0.47
Hα Broad42.26 ± 0.011989 ± 661221 ± 25366.30 ± 1.14
[N II] 658541.22 ± 0.01526 ± 63223 ± 2533.86 ± 0.43
[S II] 671840.63 ± 0.03526 ± 63223 ± 258.86 ± 0.35
[S II] 673240.48 ± 0.04526 ± 63223 ± 256.18 ± 0.35

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 SNR28.08
Hβ Broad SNR5.55
Hγ Broad SNR1.48
AGN frac0.34
Host frac0.66
log L5100,Host43.75
Fe II/Hβ1.64
Fe II/[O III]3.91

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr1
hb_width2
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.