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LEDA 3082029

Observation

Spectrum ID104137171_sp1
Alt nameg1235403-210248
z0.0617
RA, Dec188.9182, -21.0467
MJD60081.5
SNR/Å B/R15.9/24.7
Obs Airmass1.04
SMSS ID104137171
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.5 ± 0.1
2MASS Kext12.2 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.056
Power law αν-0.14 ± 0.15
log L5100,AGN43.29 ± 0.02
log HβBr/[O III]0.06 ± 0.02
log ML5100/M7.32 ± 0.08
log M/M6.97 ± 0.03
log M/M7.25 ± 0.09
log M[O III]/M7.36 ± 0.08

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 Narrow39.78 ± 0.22369 ± 63237 ± 261.17 ± 0.35
Hγ Broad40.76 ± 0.073502 ± 3271311 ± 9110.88 ± 0.92
[O III] 436439.65 ± 0.18271 ± 63114 ± 250.88 ± 0.23
He II Narrow39.79 ± 0.12271 ± 63114 ± 251.37 ± 0.25
He II Broad40.62 ± 0.084354 ± 3711849 ± 1579.27 ± 0.99
Hβ Narrow40.47 ± 0.06369 ± 63237 ± 267.13 ± 0.40
Hβ Broad41.32 ± 0.022301 ± 2121704 ± 8849.77 ± 1.34
[O III] 500741.26 ± 0.01369 ± 63237 ± 2646.00 ± 0.45
He I Narrow38.95 ± 0.40271 ± 63114 ± 250.31 ± 0.28
He I Broad40.79 ± 0.043317 ± 1641409 ± 6920.79 ± 1.04
[O I] 630039.83 ± 0.07271 ± 63114 ± 252.64 ± 0.29
Hα Narrow40.86 ± 0.01271 ± 63114 ± 2530.44 ± 0.43
Hα Broad41.82 ± 0.011933 ± 71995 ± 26278.00 ± 1.48
[N II] 658540.72 ± 0.01271 ± 63114 ± 2522.08 ± 0.37
[S II] 671840.29 ± 0.03271 ± 63114 ± 258.43 ± 0.35
[S II] 673240.16 ± 0.03271 ± 63114 ± 256.38 ± 0.34

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 SNR21.57
Hβ Broad SNR6.34
Hγ Broad SNR1.89
AGN frac0.49
Host frac0.51
log L5100,Host43.31
Fe II/Hβ0.93
Fe II/[O III]1.06

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr1
hb_width2
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.