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LEDA 835095

Observation

Spectrum ID172750140_sp1
Alt nameg1638309-205525
z0.0270
RA, Dec249.6288, -20.9235
MJD60160.41
SNR/Å B/R11.8/15.3
Obs Airmass1.02
SMSS ID172750140
Closest SMSS2.67'', 2259513749
SMSS Mean r6"ap15.4 ± 0.0
2MASS Kext11.0 ± 0.0

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.429
Power law αν-0.88 ± 0.04
log L5100,AGN43.60 ± 0.01
log HβBr/[O III]0.16 ± 0.05
log ML5100/M7.39 ± 0.10
log M/M6.92 ± 0.04
log M/M7.38 ± 0.11
log M[O III]/M7.46 ± 0.10

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 Narrow40.65 ± 0.12446 ± 63311 ± 294.73 ± 0.39
Hγ Broad41.42 ± 0.032523 ± 4631099 ± 19027.80 ± 0.77
[O III] 436439.75 ± 0.33357 ± 66150 ± 270.60 ± 0.24
He II Narrow39.85 ± 0.21357 ± 66150 ± 270.83 ± 0.23
He II Broad41.25 ± 0.083481 ± 6021478 ± 25520.57 ± 0.71
Hβ Narrow40.98 ± 0.07446 ± 63311 ± 2911.55 ± 0.38
Hβ Broad41.75 ± 0.052132 ± 263978 ± 19768.18 ± 0.80
[O III] 500741.59 ± 0.01446 ± 63311 ± 2948.09 ± 0.39
He I Narrow39.81 ± 0.20357 ± 66150 ± 270.96 ± 0.17
He I Broad40.78 ± 0.091982 ± 566841 ± 2409.08 ± 0.43
[O I] 630039.79 ± 0.15357 ± 66150 ± 271.01 ± 0.21
Hα Narrow40.93 ± 0.05357 ± 66150 ± 2714.22 ± 0.38
Hα Broad42.19 ± 0.011408 ± 67703 ± 32265.50 ± 0.76
[N II] 658540.92 ± 0.04357 ± 66150 ± 2713.92 ± 0.32
[S II] 671840.38 ± 0.04357 ± 66150 ± 274.19 ± 0.23
[S II] 673240.35 ± 0.04357 ± 66150 ± 273.94 ± 0.23

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 SNR48.54
Hβ Broad SNR16.11
Hγ Broad SNR7.53
AGN frac0.99
Host frac0.01
log L5100,Host41.61
Fe II/Hβ0.74
Fe II/[O III]1.09

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.