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LEDA 152500

Observation

Spectrum ID75828917_sp1
Alt nameg0827341-021247
z0.0394
RA, Dec126.8923, -2.2130
MJD60021.44
SNR/Å B/R14.2/36.7
Obs Airmass1.14
SMSS ID75828917
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.9 ± 0.0
2MASS Kext11.7 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.027
Power law αν-0.45 ± 0.37
log L5100,AGN42.68 ± 0.06
log HβBr/[O III]0.11 ± 0.04
log ML5100/M7.26 ± 0.07
log M/M6.80 ± 0.04
log M/M7.24 ± 0.08
log M[O III]/M7.31 ± 0.07

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 Narrow39.44 ± 0.28273 ± 63211 ± 282.27 ± 1.04
Hγ Broad40.38 ± 0.081943 ± 273726 ± 7218.61 ± 2.00
[O III] 436439.25 ± 0.27238 ± 63100 ± 251.49 ± 0.62
He II Narrow39.23 ± 0.24238 ± 63100 ± 251.59 ± 0.59
He II Broad40.64 ± 0.068372 ± 1153555 ± 4840.81 ± 3.52
Hβ Narrow39.89 ± 0.08273 ± 63211 ± 287.56 ± 0.98
Hβ Broad40.86 ± 0.032882 ± 1971415 ± 11670.33 ± 3.06
[O III] 500740.75 ± 0.01273 ± 63211 ± 2858.08 ± 1.07
He I Narrow38.61 ± 0.36238 ± 63100 ± 250.54 ± 0.36
He I Broad40.41 ± 0.056922 ± 1892939 ± 8033.81 ± 2.18
[O I] 630039.39 ± 0.09238 ± 63100 ± 253.58 ± 0.41
Hα Narrow40.22 ± 0.02238 ± 63100 ± 2526.00 ± 0.50
Hα Broad41.36 ± 0.012202 ± 68991 ± 27361.52 ± 2.22
[N II] 658540.33 ± 0.01238 ± 63100 ± 2533.74 ± 0.51
[S II] 671839.87 ± 0.03238 ± 63100 ± 2512.19 ± 0.51
[S II] 673239.77 ± 0.03238 ± 63100 ± 259.64 ± 0.49

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 SNR12.78
Hβ Broad SNR3.93
Hγ Broad SNR2.54
AGN frac0.22
Host frac0.78
log L5100,Host43.22
Fe II/Hβ0.44
Fe II/[O III]0.55

Quality flags

spurious_hab/hbb0.0/0
l51001
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.