← atlas

LEDA 2816917

Observation

Spectrum ID308745927_sp1
Alt nameg1438031-450146
z0.0740
RA, Dec219.5128, -45.0294
MJD60055.61
SNR/Å B/R13.6/16.9
Obs Airmass1.03
SMSS ID308745927
Closest SMSS0.87'', 2458118525
SMSS Mean r6"ap16.7 ± 0.1
2MASS Kext13.3 ± 0.2

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.133
Power law αν-1.05 ± 0.05
log L5100,AGN43.59 ± 0.01
log HβBr/[O III]-0.20 ± 0.03
log ML5100/M7.49 ± 0.04
log M/M6.99 ± 0.04
log M/M7.39 ± 0.04
log M[O III]/M7.64 ± 0.03

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 Narrow40.18 ± 0.14342 ± 63175 ± 251.71 ± 0.24
Hγ Broad40.98 ± 0.061784 ± 431984 ± 8711.05 ± 0.67
[O III] 436439.91 ± 0.17316 ± 63133 ± 250.94 ± 0.25
He II Narrow40.09 ± 0.09316 ± 63133 ± 251.49 ± 0.20
He II Broad40.77 ± 0.096345 ± 2322694 ± 987.24 ± 0.90
Hβ Narrow40.79 ± 0.03342 ± 63175 ± 257.82 ± 0.24
Hβ Broad41.54 ± 0.032397 ± 932540 ± 12243.71 ± 1.43
[O III] 500741.75 ± 0.01342 ± 63175 ± 2572.25 ± 0.30
He I Narrow39.64 ± 0.22316 ± 63133 ± 250.66 ± 0.25
He I Broad40.49 ± 0.092453 ± 1981041 ± 844.82 ± 0.55
[O I] 630040.46 ± 0.03316 ± 63133 ± 254.67 ± 0.19
Hα Narrow41.26 ± 0.01316 ± 63133 ± 2530.26 ± 0.26
Hα Broad41.91 ± 0.011874 ± 75830 ± 25135.73 ± 0.65
[N II] 658541.11 ± 0.01316 ± 63133 ± 2521.53 ± 0.24
[S II] 671840.79 ± 0.01316 ± 63133 ± 2510.56 ± 0.22
[S II] 673240.72 ± 0.02316 ± 63133 ± 259.11 ± 0.28

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 SNR21.49
Hβ Broad SNR6.61
Hγ Broad SNR3.62
AGN frac0.85
Host frac0.15
log L5100,Host42.83
Fe II/Hβ0.46
Fe II/[O III]0.28

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
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.