← atlas

LEDA 3095437

Observation

Spectrum ID491314147_sp1
Alt namePGC 3095437
z0.0744
RA, Dec8.5700, -79.0890
MJD60931.57
SNR/Å B/R6.6/9.2
Obs Airmass1.51
SMSS ID491314147
Closest SMSS13.35'', 491314145
SMSS Mean r6"ap15.0 ± 0.0
2MASS Kext11.6 ± 0.0

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN referencePGC
MW E(B−V)0.070
Power law αν0.12 ± 0.20
log L5100,AGN44.21 ± 0.03
log HβBr/[O III]0.30 ± 0.08
log ML5100/M7.80 ± 0.08
log M/M7.83 ± 0.11
log M/M7.86 ± 0.09
log M[O III]/M7.91 ± 0.09

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 Narrow41.16 ± 0.26466 ± 124292 ± 702.95 ± 0.73
Hγ Broad41.98 ± 0.081802 ± 415593 ± 14019.06 ± 1.07
[O III] 436441.04 ± 0.36404 ± 111170 ± 462.76 ± 0.49
He II Narrow40.66 ± 0.42404 ± 111170 ± 461.39 ± 0.46
He II Broad41.31 ± 0.151425 ± 139605 ± 585.42 ± 0.89
Hβ Narrow41.47 ± 0.14466 ± 124292 ± 707.39 ± 0.84
Hβ Broad42.51 ± 0.052519 ± 230834 ± 11883.83 ± 1.38
[O III] 500742.21 ± 0.06466 ± 124292 ± 7048.04 ± 0.91
He I Narrow40.54 ± 0.34404 ± 111170 ± 461.61 ± 0.53
He I Broad41.30 ± 0.211658 ± 394704 ± 1678.62 ± 1.03
[O I] 630040.63 ± 0.21404 ± 111170 ± 462.23 ± 0.50
Hα Narrow41.93 ± 0.19404 ± 111170 ± 4651.00 ± 1.18
Hα Broad43.06 ± 0.022196 ± 268972 ± 107637.29 ± 2.32
[N II] 658541.41 ± 0.22404 ± 111170 ± 4613.78 ± 1.04
[S II] 671841.18 ± 0.09404 ± 111170 ± 469.17 ± 0.66
[S II] 673241.21 ± 0.12404 ± 111170 ± 469.44 ± 0.83

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 SNR27.46
Hβ Broad SNR10.17
Hγ Broad SNR4.58
AGN frac0.83
Host frac0.16
log L5100,Host43.50
Fe II/Hβ0.62
Fe II/[O III]1.15

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
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.