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LEDA 1029293

Observation

Spectrum ID169046541_sp1
Alt nameg1522287-064441
z0.0833
RA, Dec230.6196, -6.7447
MJD60080.58
SNR/Å B/R14.8/17.8
Obs Airmass1.10
SMSS ID169046541
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.2 ± 0.1
2MASS Kext12.3 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.082
Power law αν-0.06 ± 0.13
log L5100,AGN43.81 ± 0.02
log HβBr/[O III]0.28 ± 0.02
log ML5100/M7.09 ± 0.02
log M/M7.11 ± 0.05
log M/M7.11 ± 0.02
log M[O III]/M7.14 ± 0.02

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 Narrow40.99 ± 0.14666 ± 66505 ± 265.62 ± 0.46
Hγ Broad41.50 ± 0.061287 ± 78623 ± 8818.41 ± 0.75
[O III] 436440.26 ± 0.20494 ± 64209 ± 261.05 ± 0.28
He II Narrow40.11 ± 0.21494 ± 64209 ± 260.86 ± 0.27
He II Broad41.24 ± 0.087506 ± 3083187 ± 13011.69 ± 1.12
Hβ Narrow41.41 ± 0.07666 ± 66505 ± 2618.45 ± 0.54
Hβ Broad42.04 ± 0.021353 ± 30921 ± 3678.42 ± 1.03
[O III] 500741.75 ± 0.01666 ± 66505 ± 2643.41 ± 0.64
He I Narrow40.35 ± 0.14494 ± 64209 ± 262.31 ± 0.36
He I Broad41.30 ± 0.032864 ± 1361216 ± 5721.00 ± 0.88
[O I] 630040.56 ± 0.07494 ± 64209 ± 264.33 ± 0.42
Hα Narrow41.73 ± 0.03494 ± 64209 ± 2669.39 ± 0.61
Hα Broad42.54 ± 0.011378 ± 66716 ± 25442.96 ± 1.41
[N II] 658541.32 ± 0.02494 ± 64209 ± 2627.04 ± 0.54
[S II] 671840.91 ± 0.04494 ± 64209 ± 2610.81 ± 0.62
[S II] 673240.85 ± 0.03494 ± 64209 ± 269.60 ± 0.67

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 SNR55.12
Hβ Broad SNR21.02
Hγ Broad SNR8.43
AGN frac0.70
Host frac0.30
log L5100,Host43.45
Fe II/Hβ1.00
Fe II/[O III]1.91

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width1
balmer_width1

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.