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LAMOST J124059.02-060753.4

Observation

Spectrum ID106849647_sp1
Alt nameg1240590-060753
z0.0498
RA, Dec190.2458, -6.1315
MJD59016.4
SNR/Å B/R22.3/34.2
Obs Airmass1.11
SMSS ID106849647
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.2 ± 0.0
2MASS Kext12.6 ± 0.1

AGN Properties

Spectrum TypeSy 1.8
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.021
Power law αν0.12 ± 0.10
log L5100,AGN43.22 ± 0.02
log HβBr/[O III]-0.73 ± 0.08
log ML5100/M7.74 ± 0.19
log M/M6.52 ± 0.05
log M/M7.30 ± 0.20
log M[O III]/M7.77 ± 0.19

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 Narrow40.06 ± 0.06209 ± 63196 ± 252.50 ± 0.24
Hγ Broad40.25 ± 0.091204 ± 66713 ± 1873.80 ± 0.47
[O III] 436438.90 ± 0.40189 ± 6277 ± 250.18 ± 0.13
He II Narrow39.59 ± 0.10189 ± 6277 ± 250.99 ± 0.13
He II Broad40.21 ± 0.102840 ± 1671206 ± 704.31 ± 0.55
Hβ Narrow40.49 ± 0.02209 ± 63196 ± 258.55 ± 0.27
Hβ Broad40.44 ± 0.083850 ± 8351672 ± 967.33 ± 0.74
[O III] 500741.17 ± 0.01209 ± 63196 ± 2543.63 ± 0.30
He I Narrow39.09 ± 0.20189 ± 6277 ± 250.51 ± 0.14
He I Broad40.08 ± 0.093123 ± 1131326 ± 474.86 ± 0.56
[O I] 630039.50 ± 0.07189 ± 6277 ± 251.51 ± 0.15
Hα Narrow40.84 ± 0.01189 ± 6277 ± 2536.07 ± 0.25
Hα Broad41.33 ± 0.011630 ± 711345 ± 28110.24 ± 1.09
[N II] 658540.53 ± 0.01189 ± 6277 ± 2517.92 ± 0.22
[S II] 671840.15 ± 0.02189 ± 6277 ± 257.78 ± 0.22
[S II] 673240.07 ± 0.02189 ± 6277 ± 256.42 ± 0.19

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 SNR10.98
Hβ Broad SNR1.23
Hγ Broad SNR2.56
AGN frac0.49
Host frac0.51
log L5100,Host43.24
Fe II/Hβ0.85
Fe II/[O III]0.15

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer1
balmer_snr2
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.