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LEDA 596567

Observation

Spectrum ID1705936_sp2
Alt nameg2245238-393441
z0.0983
RA, Dec341.3493, -39.5779
MJD60114.79
SNR/Å B/R8.9/10.8
Obs Airmass1.01
SMSS ID1705936
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.5 ± 0.1
2MASS Kext12.8 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.011
Power law αν0.10 ± 0.31
log L5100,AGN43.32 ± 0.06
log HβBr/[O III]0.46 ± 0.03
log ML5100/M7.80 ± 0.07
log M/M7.73 ± 0.04
log M/M8.02 ± 0.06
log M[O III]/M7.96 ± 0.06

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 Narrow39.81 ± 0.40480 ± 63206 ± 261.12 ± 0.84
Hγ Broad41.18 ± 0.073134 ± 2291144 ± 4926.15 ± 2.00
[O III] 436439.96 ± 0.34477 ± 63202 ± 251.62 ± 0.73
He II Narrow40.05 ± 0.27477 ± 63202 ± 252.31 ± 0.79
He II Broad39.84 ± 0.461205 ± 69512 ± 281.39 ± 1.22
Hβ Narrow40.47 ± 0.13480 ± 63206 ± 266.51 ± 1.08
Hβ Broad41.99 ± 0.023924 ± 2624116 ± 90219.68 ± 5.86
[O III] 500741.53 ± 0.01480 ± 63206 ± 2680.44 ± 1.43
He I Narrow39.96 ± 0.25477 ± 63202 ± 253.01 ± 1.15
He I Broad41.55 ± 0.0512257 ± 935205 ± 38116.68 ± 6.22
[O I] 630040.20 ± 0.18477 ± 63202 ± 256.11 ± 1.50
Hα Narrow41.16 ± 0.03477 ± 63202 ± 2560.94 ± 1.80
Hα Broad42.35 ± 0.013216 ± 1211743 ± 26940.71 ± 6.64
[N II] 658541.42 ± 0.02477 ± 63202 ± 25111.57 ± 2.39
[S II] 671840.82 ± 0.04477 ± 63202 ± 2529.47 ± 2.18
[S II] 673240.83 ± 0.05477 ± 63202 ± 2530.22 ± 2.09

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 SNR15.35
Hβ Broad SNR5.07
Hγ Broad SNR1.98
AGN frac0.40
Host frac0.60
log L5100,Host43.49
Fe II/Hβ0.60
Fe II/[O III]1.73

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.