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NAME MR 2251-178

Observation

Spectrum ID6111939_sp1
Alt nameMR 2251-178
z0.0638
RA, Dec343.5245, -17.5820
MJD60176.61
SNR/Å B/R7.4/12.9
Obs Airmass1.04
SMSS ID6111939
Closest SMSS6.54'', 2010543874
SMSS Mean r6"ap14.2 ± 0.1
2MASS Kext11.1 ± 0.0

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.034
Power law αν-0.13 ± 0.13
log L5100,AGN43.41 ± 0.02
log HβBr/[O III]-0.03 ± 0.01
log ML5100/M7.97 ± 0.11
log M/M7.89 ± 0.03
log M/M8.13 ± 0.10
log M[O III]/M8.32 ± 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 Narrow40.39 ± 0.16474 ± 63415 ± 253.60 ± 0.81
Hγ Broad41.52 ± 0.033320 ± 1421189 ± 4148.16 ± 1.30
[O III] 436440.43 ± 0.09414 ± 63176 ± 253.99 ± 0.44
He II Narrow40.08 ± 0.16414 ± 63176 ± 252.04 ± 0.44
He II Broad40.98 ± 0.085183 ± 2062201 ± 8715.66 ± 1.64
Hβ Narrow41.05 ± 0.04474 ± 63415 ± 2520.22 ± 0.90
Hβ Broad41.97 ± 0.014560 ± 5402725 ± 60167.69 ± 2.28
[O III] 500742.00 ± 0.01474 ± 63415 ± 25189.15 ± 1.02
He I Narrow39.86 ± 0.15414 ± 63176 ± 251.85 ± 0.36
He I Broad40.77 ± 0.063561 ± 1801512 ± 7615.34 ± 1.09
[O I] 630040.55 ± 0.03414 ± 63176 ± 2510.34 ± 0.41
Hα Narrow41.23 ± 0.02414 ± 63176 ± 2553.56 ± 0.78
Hα Broad42.65 ± 0.013120 ± 701818 ± 251424.56 ± 2.17
[N II] 658540.41 ± 0.06414 ± 63176 ± 258.16 ± 0.66
[S II] 671840.52 ± 0.03414 ± 63176 ± 2510.93 ± 0.49
[S II] 673240.50 ± 0.03414 ± 63176 ± 2510.53 ± 0.50

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 SNR47.00
Hβ Broad SNR9.08
Hγ Broad SNR6.30
AGN frac0.83
Host frac0.17
log L5100,Host42.71
Fe II/Hβ0.29
Fe II/[O III]0.27

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.