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LEDA 3095695

Observation

Spectrum ID19557796_sp1
Alt namePGC 3095695
z0.0800
RA, Dec70.3439, -27.1387
MJD60946.76
SNR/Å B/R9.6/15.9
Obs Airmass1.00
SMSS ID19557796
Closest SMSS10.98'', 19557800
SMSS Mean r6"ap15.5 ± 0.0
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN referencePGC
MW E(B−V)0.031
Power law αν-1.45 ± 0.14
log L5100,AGN44.03 ± 0.02
log HβBr/[O III]-0.34 ± 0.06
log ML5100/M7.85 ± 0.15
log M/M7.87 ± 0.06
log M/M7.85 ± 0.16
log M[O III]/M8.20 ± 0.16

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 Narrow41.07 ± 0.08345 ± 63189 ± 315.12 ± 0.52
Hγ Broad41.41 ± 0.142035 ± 724619 ± 22310.07 ± 0.80
[O III] 436440.85 ± 0.17340 ± 63143 ± 253.10 ± 0.33
He II Narrow40.88 ± 0.09340 ± 63143 ± 253.42 ± 0.31
He II Broad41.14 ± 0.192013 ± 915854 ± 3884.95 ± 0.69
Hβ Narrow41.42 ± 0.05345 ± 63189 ± 3112.19 ± 0.53
Hβ Broad42.20 ± 0.062920 ± 4641400 ± 29774.29 ± 1.15
[O III] 500742.54 ± 0.01345 ± 63189 ± 31165.00 ± 0.67
He I Narrow40.30 ± 0.21340 ± 63143 ± 251.03 ± 0.20
He I Broad41.22 ± 0.142300 ± 964977 ± 4098.02 ± 0.56
[O I] 630040.86 ± 0.04340 ± 63143 ± 253.91 ± 0.21
Hα Narrow42.02 ± 0.02340 ± 63143 ± 2557.90 ± 0.42
Hα Broad42.88 ± 0.012600 ± 1491242 ± 39417.33 ± 1.02
[N II] 658541.26 ± 0.04340 ± 63143 ± 2510.14 ± 0.34
[S II] 671841.22 ± 0.02340 ± 63143 ± 259.19 ± 0.29
[S II] 673241.10 ± 0.03340 ± 63143 ± 257.01 ± 0.29

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 SNR37.82
Hβ Broad SNR9.85
Hγ Broad SNR2.80
AGN frac0.90
Host frac0.10
log L5100,Host43.07
Fe II/Hβ0.37
Fe II/[O III]0.17

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
hb_width0
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.