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LEDA 89057

Observation

Spectrum ID481135279_sp1
Alt nameg1938044-510950
z0.0403
RA, Dec294.5183, -51.1637
MJD60165.52
SNR/Å B/R13.7/20.6
Obs Airmass1.06
SMSS ID481135279
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.7 ± 0.2
2MASS Kext11.6 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.053
Power law αν-1.21 ± 0.02
log L5100,AGN43.40 ± 0.01
log HβBr/[O III]0.48 ± 0.01
log ML5100/M7.60 ± 0.03
log M/M7.44 ± 0.02
log M/M7.64 ± 0.03
log M[O III]/M7.57 ± 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 Narrow39.86 ± 0.15304 ± 63320 ± 281.29 ± 0.40
Hγ Broad41.27 ± 0.023518 ± 1151155 ± 3632.66 ± 0.59
[O III] 436439.67 ± 0.17285 ± 63121 ± 250.83 ± 0.18
He II Narrow39.48 ± 0.20285 ± 63121 ± 250.57 ± 0.17
He II Broad41.29 ± 0.027409 ± 1953146 ± 8237.09 ± 0.90
Hβ Narrow40.29 ± 0.06304 ± 63321 ± 283.76 ± 0.38
Hβ Broad41.69 ± 0.012990 ± 831492 ± 3694.42 ± 0.80
[O III] 500741.21 ± 0.01304 ± 63321 ± 2832.34 ± 0.39
He I Narrow39.47 ± 0.13285 ± 63121 ± 250.67 ± 0.12
He I Broad40.85 ± 0.023532 ± 1351500 ± 5715.81 ± 0.42
[O I] 630039.37 ± 0.15285 ± 63121 ± 250.55 ± 0.12
Hα Narrow40.76 ± 0.02285 ± 63121 ± 2514.16 ± 0.24
Hα Broad42.14 ± 0.012649 ± 661188 ± 25342.23 ± 0.68
[N II] 658540.00 ± 0.06285 ± 63121 ± 252.46 ± 0.20
[S II] 671839.96 ± 0.04285 ± 63121 ± 252.31 ± 0.14
[S II] 673239.90 ± 0.04285 ± 63121 ± 252.01 ± 0.14

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 SNR46.85
Hβ Broad SNR18.50
Hγ Broad SNR8.45
AGN frac1.00
Host frac0.00
log L5100,Host40.85
Fe II/Hβ0.17
Fe II/[O III]0.52

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
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.