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LEDA 2817164

Observation

Spectrum ID229656645_sp1
Alt nameIRAS 19370-3022
z0.0529
RA, Dec295.0629, -30.2644
MJD60905.44
SNR/Å B/R14.7/22.2
Obs Airmass1.05
SMSS ID229656645
Closest SMSS10.62'', 229656646
SMSS Mean r6"apnan ± nan
2MASS Kext11.3 ± 0.0

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN referencePGC
MW E(B−V)0.088
Power law αν-1.20 ± 0.02
log L5100,AGN44.05 ± 0.01
log HβBr/[O III]0.55 ± 0.01
log ML5100/M8.23 ± 0.02
log M/M8.10 ± 0.03
log M/M8.28 ± 0.02
log M[O III]/M8.19 ± 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 Narrow40.48 ± 0.13342 ± 63146 ± 251.19 ± 0.25
Hγ Broad41.96 ± 0.034675 ± 3353402 ± 11036.63 ± 1.27
[O III] 436439.82 ± 0.39342 ± 63144 ± 250.27 ± 0.19
He II Narrow40.43 ± 0.11342 ± 63144 ± 251.15 ± 0.18
He II Broad41.86 ± 0.0312928 ± 695490 ± 2830.88 ± 1.14
Hβ Narrow41.09 ± 0.03342 ± 63146 ± 255.38 ± 0.25
Hβ Broad42.32 ± 0.014476 ± 1143041 ± 5591.13 ± 1.15
[O III] 500741.76 ± 0.01342 ± 63146 ± 2525.88 ± 0.27
He I Narrow40.21 ± 0.10342 ± 63144 ± 250.82 ± 0.12
He I Broad41.49 ± 0.035765 ± 952448 ± 3915.58 ± 0.53
[O I] 630040.57 ± 0.04342 ± 63144 ± 252.01 ± 0.13
Hα Narrow41.69 ± 0.01342 ± 63144 ± 2527.44 ± 0.25
Hα Broad42.72 ± 0.013763 ± 661752 ± 27293.96 ± 0.88
[N II] 658541.45 ± 0.01342 ± 63144 ± 2515.59 ± 0.23
[S II] 671840.95 ± 0.02342 ± 63144 ± 255.07 ± 0.15
[S II] 673240.89 ± 0.02342 ± 63144 ± 254.40 ± 0.15

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 SNR29.67
Hβ Broad SNR10.88
Hγ Broad SNR4.91
AGN frac1.00
Host frac0.00
log L5100,Host41.52
Fe II/Hβ0.29
Fe II/[O III]1.03

Quality flags

spurious_hab/hbb0.0/0
l51000
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.