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2MASS J16161077-1014059

Observation

Spectrum ID192188594_sp2
Alt nameg1616108-101406
z0.0767
RA, Dec244.0449, -10.2350
MJD59671.7
SNR/Å B/R9.2/14.6
Obs Airmass1.09
SMSS ID192188594
Closest SMSS13.95'', 192188595
SMSS Mean r6"ap17.4 ± 0.1
2MASS Kext12.6 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.234
Power law αν-0.23 ± 0.32
log L5100,AGN43.32 ± 0.05
log HβBr/[O III]0.20 ± 0.02
log ML5100/M7.34 ± 0.07
log M/M7.11 ± 0.03
log M/M7.43 ± 0.06
log M[O III]/M7.49 ± 0.06

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 Narrow40.09 ± 0.25316 ± 63326 ± 292.25 ± 1.00
Hγ Broad41.19 ± 0.042475 ± 171844 ± 4328.66 ± 1.19
[O III] 436439.93 ± 0.26300 ± 63127 ± 251.58 ± 0.48
He II Narrow40.19 ± 0.10300 ± 63127 ± 253.29 ± 0.50
He II Broad41.38 ± 0.0615475 ± 2756572 ± 11650.81 ± 3.81
Hβ Narrow40.55 ± 0.08316 ± 63326 ± 298.02 ± 1.13
Hβ Broad41.70 ± 0.012312 ± 1611196 ± 45113.65 ± 2.03
[O III] 500741.51 ± 0.01316 ± 63326 ± 2976.54 ± 1.31
He I Narrow39.21 ± 0.41300 ± 63127 ± 250.51 ± 0.43
He I Broad40.53 ± 0.082053 ± 160872 ± 6710.72 ± 1.18
[O I] 630039.49 ± 0.25300 ± 63127 ± 251.12 ± 0.45
Hα Narrow40.86 ± 0.02300 ± 63127 ± 2527.73 ± 0.64
Hα Broad42.13 ± 0.011843 ± 66850 ± 25513.26 ± 2.08
[N II] 658540.68 ± 0.03300 ± 63127 ± 2518.50 ± 0.60
[S II] 671840.38 ± 0.04300 ± 63127 ± 259.66 ± 0.75
[S II] 673240.26 ± 0.06300 ± 63127 ± 257.33 ± 0.78

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 SNR25.90
Hβ Broad SNR10.04
Hγ Broad SNR4.35
AGN frac0.50
Host frac0.50
log L5100,Host43.31
Fe II/Hβ0.50
Fe II/[O III]0.78

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.