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2MASS J15080462-4244448

Observation

Spectrum ID310181797_sp2
Alt nameg1508046-424445
z0.0562
RA, Dec227.0190, -42.7458
MJD59671.64
SNR/Å B/R11.9/22.3
Obs Airmass1.05
SMSS ID310181797
Closest SMSS5.01'', 2460485054
SMSS Mean r6"ap16.4 ± 0.1
2MASS Kext12.5 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.106
Power law αν-0.94 ± 0.18
log L5100,AGN43.35 ± 0.03
log HβBr/[O III]0.12 ± 0.02
log ML5100/M7.82 ± 0.05
log M/M7.15 ± 0.04
log M/M7.78 ± 0.06
log M[O III]/M7.87 ± 0.05

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 Narrow39.96 ± 0.20355 ± 63303 ± 381.75 ± 0.65
Hγ Broad41.01 ± 0.053823 ± 4031333 ± 7920.08 ± 1.19
[O III] 436439.35 ± 0.40337 ± 63143 ± 250.43 ± 0.34
He II Narrow39.76 ± 0.18337 ± 63143 ± 251.18 ± 0.34
He II Broad40.99 ± 0.0710283 ± 2894367 ± 12220.18 ± 1.89
Hβ Narrow40.53 ± 0.05355 ± 63303 ± 387.44 ± 0.64
Hβ Broad41.45 ± 0.023979 ± 2191838 ± 8760.22 ± 1.53
[O III] 500741.32 ± 0.01355 ± 63303 ± 3847.52 ± 0.72
He I Narrow39.73 ± 0.12337 ± 63143 ± 251.40 ± 0.25
He I Broad40.67 ± 0.064416 ± 2821875 ± 11912.35 ± 0.93
[O I] 630039.88 ± 0.08337 ± 63143 ± 252.14 ± 0.26
Hα Narrow40.99 ± 0.01337 ± 63143 ± 2529.22 ± 0.37
Hα Broad41.94 ± 0.012189 ± 941434 ± 27258.77 ± 1.23
[N II] 658540.88 ± 0.01337 ± 63143 ± 2522.46 ± 0.35
[S II] 671840.37 ± 0.03337 ± 63143 ± 257.12 ± 0.31
[S II] 673240.29 ± 0.03337 ± 63143 ± 255.94 ± 0.30

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 SNR18.05
Hβ Broad SNR5.11
Hγ Broad SNR2.64
AGN frac0.58
Host frac0.42
log L5100,Host43.22
Fe II/Hβ0.36
Fe II/[O III]0.47

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
hb_width0
balmer_width1

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.