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LEDA 84945

Observation

Spectrum ID487995745_sp1
Alt nameg2049332-390204
z0.0411
RA, Dec312.3882, -39.0343
MJD59438.46
SNR/Å B/R12.0/27.6
Obs Airmass1.18
SMSS ID487995745
Closest SMSS7.95'', 1596138593
SMSS Mean r6"ap16.4 ± 0.0
2MASS Kext13.1 ± 0.1

AGN Properties

Spectrum TypeSy 1.8
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.040
Power law αν-1.72 ± 0.07
log L5100,AGN42.62 ± 0.03
log HβBr/[O III]-0.80 ± 0.03
log ML5100/M6.85 ± 0.15
log M/M6.50 ± 0.05
log M/M6.79 ± 0.16
log M[O III]/M7.30 ± 0.15

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 Narrow40.09 ± 0.08379 ± 62309 ± 2514.26 ± 1.47
Hγ Broad39.93 ± 0.181316 ± 141511 ± 788.57 ± 1.85
[O III] 436439.79 ± 0.08342 ± 62144 ± 257.10 ± 0.82
He II Narrow39.79 ± 0.07342 ± 62144 ± 257.36 ± 0.73
He II Broad40.49 ± 0.054073 ± 701730 ± 2836.10 ± 2.48
Hβ Narrow40.55 ± 0.03379 ± 62309 ± 2542.55 ± 1.23
Hβ Broad40.71 ± 0.031850 ± 2991524 ± 7461.13 ± 2.78
[O III] 500741.52 ± 0.01379 ± 62309 ± 25395.11 ± 1.40
He I Narrow39.13 ± 0.21342 ± 62144 ± 251.71 ± 0.36
He I Broad40.01 ± 0.051179 ± 62500 ± 2512.91 ± 0.69
[O I] 630040.04 ± 0.02342 ± 62144 ± 2514.12 ± 0.38
Hα Narrow40.93 ± 0.01342 ± 62144 ± 25111.36 ± 0.50
Hα Broad41.39 ± 0.011527 ± 66720 ± 25316.63 ± 1.29
[N II] 658540.64 ± 0.01342 ± 62144 ± 2557.14 ± 0.50
[S II] 671840.44 ± 0.01342 ± 62144 ± 2536.04 ± 0.41
[S II] 673240.43 ± 0.01342 ± 62144 ± 2535.01 ± 0.40

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 SNR23.70
Hβ Broad SNR4.03
Hγ Broad SNR1.57
AGN frac0.30
Host frac0.70
log L5100,Host43.00
Fe II/Hβ0.38
Fe II/[O III]0.06

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.