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LEDA 3095849

Observation

Spectrum ID89191150_sp1
Alt nameg0902336-070004
z0.0898
RA, Dec135.6399, -7.0012
MJD60082.37
SNR/Å B/R9.0/10.5
Obs Airmass1.16
SMSS ID89191150
Closest SMSSNone (< 15")
SMSS Mean r6"ap17.2 ± 0.1
2MASS Kext13.5 ± 0.2

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.031
Power law αν0.35 ± 0.12
log L5100,AGN43.46 ± 0.02
log HβBr/[O III]0.54 ± 0.03
log ML5100/M7.45 ± 0.05
log M/M7.27 ± 0.04
log M/M7.54 ± 0.05
log M[O III]/M7.44 ± 0.05

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 Narrow39.88 ± 0.38312 ± 64472 ± 320.92 ± 0.73
Hγ Broad41.33 ± 0.031988 ± 218803 ± 6126.58 ± 1.07
[O III] 436439.66 ± 0.38294 ± 63123 ± 250.56 ± 0.41
He II Narrow39.58 ± 0.37294 ± 63123 ± 250.55 ± 0.33
He II Broad40.91 ± 0.081977 ± 377839 ± 16011.10 ± 0.91
Hβ Narrow40.53 ± 0.11312 ± 64473 ± 325.37 ± 0.83
Hβ Broad41.86 ± 0.022441 ± 1341264 ± 111113.03 ± 2.08
[O III] 500741.32 ± 0.02312 ± 64473 ± 3235.67 ± 1.06
He I Narrow39.62 ± 0.26294 ± 63123 ± 251.04 ± 0.40
He I Broad41.02 ± 0.042374 ± 2151008 ± 9125.01 ± 1.35
[O I] 630039.84 ± 0.22294 ± 63123 ± 251.99 ± 0.65
Hα Narrow40.97 ± 0.03294 ± 63123 ± 2530.16 ± 0.71
Hα Broad42.24 ± 0.012043 ± 88964 ± 61561.63 ± 3.56
[N II] 658540.77 ± 0.05294 ± 63123 ± 2519.24 ± 0.70
[S II] 671840.16 ± 0.10294 ± 63123 ± 254.88 ± 0.94
[S II] 673240.11 ± 0.09294 ± 63123 ± 254.37 ± 0.94

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 SNR26.77
Hβ Broad SNR11.81
Hγ Broad SNR5.59
AGN frac0.72
Host frac0.28
log L5100,Host43.05
Fe II/Hβ0.61
Fe II/[O III]2.08

Quality flags

spurious_hab/hbb0.0/0
l51002
balmer0
balmer_snr0
hb_width1
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.