Table 2.
Basic information about GRG.
| Properties | Values |
|---|---|
| RA | 22 33 01.30 |
| Dec | +13 15 02.52 |
| rband (mag) | 15.04 |
| LAS (′) | 16.1 |
| Redshift (z) | 0.09956 ± 0.00383 |
| Projected Size (Mpc) | 1.83 |
 (mJy) |
3.72 ± 0.84 |
| S1400 MHz (mJy) | 231 ± 7.8 |
| S612 MHz (mJy) | 479 ± 24.3 |
| S323 MHz (mJy) | 835 ± 83.5 |
| S144 MHz (mJy) | 1487 ± 297.4 |
 (×1022 W Hz−1) |
9.30 ± 2.20 |
| P1400 MHz (×1025 W Hz−1) | 0.60 ± 0.05 |
| P612 MHz (×1025 W Hz−1) | 1.3 ± 0.12 |
| P323 MHz (×1025 W Hz−1) | 2.2 ± 0.30 |
| P144 MHz (×1025 W Hz−1) | 3.9 ± 0.82 |
 |
0.82 ± 0.18 |
| QJet (erg s−1) | 1.3 × 1043 |
Notes. RA and Dec are right ascension and declination of the host galaxy (J2000 coordinates). Sν is integrated flux density of the source and Pν is the radio power computed at frequency ν. S1400 MHz is measured from NVSS. αint is the integrated spectral index of the GRG from 144 MHz to 1400 MHz. Angular size refers to the largest angular size (LAS) of the GRG, as measured from the 3σ contour of the LOFAR image at 144 MHz, which corresponds to 0.73 mJy beam−1. The flux density and corresponding power at 1300 MHz are from GMRT L-band observations. Here the Sν ∝ ν−α convention is followed.
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