← atlas

2MASS J14072198-3120576

Observation

Spectrum ID101746230_sp2
Alt nameg1407220-312058
z0.0746
RA, Dec211.8416, -31.3494
MJD59671.61
SNR/Å B/R14.2/23.2
Obs Airmass1.02
SMSS ID101746230
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.5 ± 0.1
2MASS Kext12.9 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.054
Power law αν-0.13 ± 0.20
log L5100,AGN43.41 ± 0.03
log HβBr/[O III]0.34 ± 0.03
log ML5100/M7.30 ± 0.07
log M/M6.83 ± 0.04
log M/M7.27 ± 0.07
log M[O III]/M7.26 ± 0.07

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 Narrow40.10 ± 0.33521 ± 64410 ± 311.84 ± 0.58
Hγ Broad40.97 ± 0.071418 ± 158874 ± 14113.57 ± 1.00
[O III] 436439.49 ± 0.40461 ± 63195 ± 250.45 ± 0.33
He II Narrow39.93 ± 0.16461 ± 63195 ± 251.41 ± 0.35
He II Broad41.25 ± 0.0614400 ± 5756115 ± 24429.26 ± 2.08
Hβ Narrow40.94 ± 0.05521 ± 64410 ± 3015.60 ± 0.67
Hβ Broad41.53 ± 0.022120 ± 1661487 ± 6861.52 ± 1.38
[O III] 500741.19 ± 0.02521 ± 64410 ± 3029.46 ± 0.74
He I Narrow39.94 ± 0.10461 ± 63195 ± 252.25 ± 0.33
He I Broad40.78 ± 0.054106 ± 2611744 ± 11015.43 ± 0.93
[O I] 630039.71 ± 0.14461 ± 63195 ± 251.49 ± 0.33
Hα Narrow41.30 ± 0.02461 ± 63195 ± 2562.35 ± 0.49
Hα Broad41.98 ± 0.011473 ± 73746 ± 25304.42 ± 1.24
[N II] 658540.97 ± 0.02461 ± 63195 ± 2529.48 ± 0.46
[S II] 671840.38 ± 0.03461 ± 63195 ± 257.82 ± 0.46
[S II] 673240.38 ± 0.04461 ± 63195 ± 257.85 ± 0.49

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 SNR30.78
Hβ Broad SNR8.66
Hγ Broad SNR4.24
AGN frac0.56
Host frac0.44
log L5100,Host43.30
Fe II/Hβ1.18
Fe II/[O III]2.60

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width1
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.