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Table 2.

Multiband radio continuum emission of IRAS 04296+2923.

Epoch freq. Prog. Beam PA Fpeak Ftotal rms Reference
(″) × (″) (°) (mJy beam−1) (mJy) (mJy beam−1)
150 MHZ TGSS 252 ± 50 a
200 MHZ GLEAM 385 ± 77 a
325 MHz WNSS 320 ± 64 a
2008Jul20 1.4 GHz AM960 41.8 × 38.6 –85 120.3 135 ± 13 3.9 b
2009Aug11 1.4 GHz AM985 13.2 × 11.6 –89 111.7 132 ± 3 1.7 b
3 GHz VLASS 2.2 × 2.3 –89 33.4 64 ± 3 0.2 c
1992Jul13 5 GHz AC326 14.2 × 13.7 –84 52.1 60 ± 2 0.5 b
16 GHZ 180 × 180 20 3 d
2005Jun24 22.5 GHz AT309 0.9 × 0.3 76 3.7 23 ± 5 0.2 e
2008Jun30 43.3 GHz AT367 1.6 × 1.0 –42 8.8 13 ± 2 0.9 b
111 GHz 4.6 × 3.8 8 9.9 11 ± 2 0.7 e

Notes. Columns (2) and (3): Observed radio frequency and program. TGSS,GLEAM, and WNSS are three radio surveys by GMRT, MWA, and Westerbork array, respectively (see the text in Sect. 2.1). Columns (4) and (5): Beam FWHM of the images. Columns (6) and (7): Peak and total flux densities. Column (8): Achieved noise level for these continuum images. Column (9): Reference of the total and peak flux. a: Stein et al. 2021 (2021, VIII/104). b: this work. c: VLASS survey. d: Perrott et al. (2015). e: Meier et al. (2010).

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