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Table 2.

Parameters of the 22 GHz H2O maser features detected toward TXS 2226-184 in epoch 1998.40.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
Maser α(a) δ(a) Component Peak flux (b) Vlsr, radio (b) ΔvL (b) rms (b), (c) S/N rms SdV(b) LH2O (d)
offset offset Density (I)
(mas) (mas) (mJy beam−1) (km s−1) (km s−1) (Jy km s−1) (L)
TXS.B01 0 0 1 36.37 7395.5 ± 0.7 61.8 ± 2.6 5.3 14 (e) 3.43 2.4 ± 0.1 869 (e)
2 38.83 7391.6 ± 0.3 20.8 ± 1.7 0.9 ± 0.1
TXS.B02 +0.601 +0.800 3 13.35 7391.3 ± 1.4 39.0 ± 5.3 5.7 28 (e) 3.69 0.5 ± 0.1 632 (e)
4 14.39 7355.3 ± 4.0 121.3 ± 5.1 1.9 ± 0.1
TXS.B03 +1.602 +3.200 5 37.66 7354.2 ± 0.6 25.9 ± 1.7 5.1 7 3.31 1.39 ± 0.04 366

Notes. The columns indicate the maser feature name, right ascension offset, declination offset, identified component from the Gaussian fit, peak flux density, peak velocity (radio convention), linewidth of the maser feature, spectral noise per channel, signal-to-noise ratio, spectral noise per km s−1, integrated flux, isotropic luminosity.

(a)

No absolute positions were measured.

(b)

Gaussian fit results.

(c)

The channel width is 0.42 km s−1.

(d)

Isotropic luminosities are derived from LH2O/[L] = 0.023 × ∫S dV/[Jy km s−1] × D2/[Mpc2], where D = 107.1 Mpc (derived assuming H0 = 70 km s−1 Mpc−1, Kuo et al. 2018).

(e)

Estimated considering the sum of the two components.

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