← atlas

ATO J214.2083-11.9827

Observation

Spectrum ID108928965_sp1
Alt nameLCRS B141408.4-114506
z0.0989
RA, Dec214.2083, -11.9828
MJD61087.76
SNR/Å B/R16.8/22.1
Obs Airmass1.06
SMSS ID108928965
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.2 ± 0.3
2MASS Kext12.1 ± 0.1

AGN Properties

Spectrum TypeSy 1.0
Quality Flaggood
AGN referencePGC
MW E(B−V)0.058
Power law αν0.48 ± 0.02
log L5100,AGN44.15 ± 0.01
log HβBr/[O III]0.93 ± 0.02
log ML5100/M8.70 ± 0.04
log M/M8.47 ± 0.05
log M/M8.89 ± 0.04
log M[O III]/M8.63 ± 0.04

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 Narrow40.24 ± 0.40595 ± 64262 ± 280.41 ± 0.28
Hγ Broad42.17 ± 0.034122 ± 3732780 ± 7836.11 ± 1.02
[O III] 436440.78 ± 0.13591 ± 64250 ± 261.48 ± 0.25
He II Narrow40.47 ± 0.21591 ± 64250 ± 260.86 ± 0.26
He II Broad42.08 ± 0.0312284 ± 1025216 ± 4234.95 ± 1.28
Hβ Narrow41.01 ± 0.08595 ± 64262 ± 283.22 ± 0.37
Hβ Broad42.71 ± 0.017362 ± 3454086 ± 44166.73 ± 1.52
[O III] 500741.78 ± 0.02595 ± 64262 ± 2820.65 ± 0.44
He I Narrow40.18 ± 0.24591 ± 64250 ± 260.77 ± 0.26
He I Broad41.74 ± 0.036662 ± 732829 ± 3027.84 ± 0.94
[O I] 630040.86 ± 0.06591 ± 64250 ± 264.36 ± 0.34
Hα Narrow41.54 ± 0.03591 ± 64250 ± 2623.06 ± 0.57
Hα Broad43.11 ± 0.014407 ± 692193 ± 25858.82 ± 1.95
[N II] 658540.69 ± 0.16591 ± 64250 ± 263.34 ± 0.58
[S II] 671840.52 ± 0.13591 ± 64250 ± 262.38 ± 0.44
[S II] 673240.67 ± 0.10591 ± 64250 ± 263.35 ± 0.43

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 SNR37.13
Hβ Broad SNR11.62
Hγ Broad SNR5.80
AGN frac0.82
Host frac0.18
log L5100,Host43.50
Fe II/Hβ0.11
Fe II/[O III]0.98

Quality flags

spurious_hab/hbb0.0/0
l51002
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.