← atlas

6dFGS gJ155703.2-074134

Observation

Spectrum ID169906444_sp1
Alt nameg1557032-074134
z0.0816
RA, Dec239.2633, -7.6927
MJD60077.68
SNR/Å B/R6.8/9.3
Obs Airmass1.19
SMSS ID169906444
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.3 ± 0.0
2MASS Kext12.8 ± 0.1

AGN Properties

Spectrum TypeSy 1.0
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.151
Power law αν-0.03 ± 0.20
log L5100,AGN43.53 ± 0.03
log HβBr/[O III]0.80 ± 0.03
log ML5100/M8.21 ± 0.10
log M/M7.46 ± 0.02
log M/M8.35 ± 0.10
log M[O III]/M8.12 ± 0.10

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 Narrow40.33 ± 0.18349 ± 64137 ± 252.38 ± 0.44
Hγ Broad40.69 ± 0.161343 ± 113514 ± 394.49 ± 0.97
[O III] 436440.10 ± 0.21265 ± 63112 ± 251.41 ± 0.42
He II Narrow39.75 ± 0.35265 ± 63112 ± 250.73 ± 0.43
He II Broad41.22 ± 0.098591 ± 663648 ± 2721.41 ± 2.62
Hβ Narrow40.54 ± 0.09349 ± 64137 ± 254.82 ± 0.49
Hβ Broad42.02 ± 0.025662 ± 6004458 ± 85145.83 ± 3.95
[O III] 500741.22 ± 0.02349 ± 64137 ± 2524.08 ± 0.58
He I Narrow39.44 ± 0.42265 ± 63112 ± 250.56 ± 0.44
He I Broad40.88 ± 0.083057 ± 711298 ± 2915.11 ± 1.62
[O I] 630039.87 ± 0.19265 ± 63112 ± 251.72 ± 0.48
Hα Narrow41.13 ± 0.02265 ± 63112 ± 2534.00 ± 0.60
Hα Broad41.95 ± 0.013101 ± 811147 ± 25223.98 ± 2.13
[N II] 658541.00 ± 0.02265 ± 63112 ± 2524.88 ± 0.60
[S II] 671840.49 ± 0.05265 ± 63112 ± 258.09 ± 0.73
[S II] 673240.34 ± 0.08265 ± 63112 ± 255.73 ± 0.77

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 SNR7.51
Hβ Broad SNR4.15
Hγ Broad SNR1.40
AGN frac0.77
Host frac0.23
log L5100,Host43.00
Fe II/Hβ0.33
Fe II/[O III]2.08

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer2
balmer_snr1
hb_width2
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.