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LEDA 433346

Observation

Spectrum ID503301360_sp1
Alt nameg0026407-530948
z0.0628
RA, Dec6.6694, -53.1633
MJD60165.75
SNR/Å B/R12.6/24.4
Obs Airmass1.09
SMSS ID503301360
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.9 ± 0.1
2MASS Kext12.1 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.017
Power law αν-0.49 ± 0.29
log L5100,AGN43.14 ± 0.05
log HβBr/[O III]0.38 ± 0.02
log ML5100/M7.80 ± 0.04
log M/M7.66 ± 0.03
log M/M8.03 ± 0.03
log M[O III]/M8.00 ± 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 Narrow39.96 ± 0.23404 ± 63310 ± 302.63 ± 1.18
Hγ Broad41.16 ± 0.053320 ± 5691417 ± 7341.53 ± 2.21
[O III] 436439.81 ± 0.25386 ± 63164 ± 251.88 ± 0.64
He II Narrow39.42 ± 0.39386 ± 63164 ± 250.86 ± 0.63
He II Broad40.71 ± 0.126181 ± 1292625 ± 5416.64 ± 2.59
Hβ Narrow40.55 ± 0.06404 ± 63311 ± 3012.12 ± 1.28
Hβ Broad41.86 ± 0.024268 ± 1173555 ± 108245.67 ± 6.06
[O III] 500741.47 ± 0.01404 ± 63311 ± 30106.01 ± 1.45
He I Narrow39.84 ± 0.13386 ± 63164 ± 253.16 ± 0.62
He I Broad41.24 ± 0.0410118 ± 1834297 ± 7779.10 ± 3.38
[O I] 630040.24 ± 0.05386 ± 63164 ± 258.80 ± 0.66
Hα Narrow40.95 ± 0.02386 ± 63164 ± 2548.00 ± 1.09
Hα Broad42.39 ± 0.012895 ± 691488 ± 251306.21 ± 3.18
[N II] 658540.93 ± 0.02386 ± 63164 ± 2545.79 ± 0.99
[S II] 671840.51 ± 0.03386 ± 63164 ± 2518.01 ± 0.76
[S II] 673240.41 ± 0.03386 ± 63164 ± 2514.35 ± 0.77

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 SNR36.05
Hβ Broad SNR7.80
Hγ Broad SNR3.27
AGN frac0.29
Host frac0.71
log L5100,Host43.53
Fe II/Hβ0.35
Fe II/[O III]0.84

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr0
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.