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LEDA 929778

Observation

Spectrum ID91196205_sp1
Alt nameg1046171-140228
z0.0677
RA, Dec161.5713, -14.0410
MJD60352.64
SNR/Å B/R16.7/23.2
Obs Airmass1.05
SMSS ID91196205
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.2 ± 0.1
2MASS Kext12.4 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.052
Power law αν-0.13 ± 0.22
log L5100,AGN43.41 ± 0.05
log HβBr/[O III]0.58 ± 0.03
log ML5100/M7.48 ± 0.05
log M/M7.14 ± 0.03
log M/M7.46 ± 0.05
log M[O III]/M7.34 ± 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 Narrow40.00 ± 0.28439 ± 63347 ± 491.48 ± 0.62
Hγ Broad40.95 ± 0.062172 ± 612951 ± 7113.30 ± 0.90
[O III] 436439.74 ± 0.31423 ± 63179 ± 250.82 ± 0.43
He II Narrow39.66 ± 0.26423 ± 63179 ± 250.77 ± 0.34
He II Broad41.16 ± 0.058935 ± 2673794 ± 11324.80 ± 1.58
Hβ Narrow40.49 ± 0.08439 ± 63347 ± 485.59 ± 0.63
Hβ Broad41.56 ± 0.022606 ± 1181641 ± 5866.18 ± 1.49
[O III] 500740.98 ± 0.03439 ± 63347 ± 4818.55 ± 0.68
He I Narrow39.50 ± 0.31423 ± 63179 ± 250.83 ± 0.38
He I Broad40.71 ± 0.073229 ± 1831371 ± 7713.29 ± 1.14
[O I] 630039.58 ± 0.23423 ± 63179 ± 251.14 ± 0.41
Hα Narrow41.20 ± 0.02423 ± 63179 ± 2551.25 ± 0.63
Hα Broad41.86 ± 0.012290 ± 711019 ± 49229.56 ± 2.32
[N II] 658541.03 ± 0.02423 ± 63179 ± 2534.09 ± 0.61
[S II] 671840.48 ± 0.04423 ± 63179 ± 2510.12 ± 0.62
[S II] 673240.28 ± 0.07423 ± 63179 ± 256.34 ± 0.65

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 SNR15.31
Hβ Broad SNR7.53
Hγ Broad SNR3.17
AGN frac0.45
Host frac0.55
log L5100,Host43.49
Fe II/Hβ0.61
Fe II/[O III]2.30

Quality flags

spurious_hab/hbb0.0/0
l51001
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.