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Table A.3.
Measurements of the cosmic radio dipole in terms of the TGSS-ADR1 from the literature.
Survey | ν | Reference | Estimator | S | N | RA | Dec | d |
---|---|---|---|---|---|---|---|---|
(MHz) | (mJy) | (deg) | (deg) | ( × 10−2) | ||||
TGSS | 147 | B18 | Hemispheres | 100 < S < 5000 | 233 395 | 155 ± 12 | 0 ± 3 | 7.0 ± 0.4 |
S19 | Source counts | S ≥ 100 | 227 773 | 162 ± 9 | 3 ± 8 | 4.42 ± 0.37 | ||
S19 | Source counts | S ≥ 150 | 161 664 | 164 ± 9 | −1 ± 8 | 4.65 ± 0.42 | ||
S19 | Source counts | S ≥ 200 | 124 080 | 166 ± 10 | −3 ± 9 | 4.65 ± 0.45 | ||
S19 | Source counts | S ≥ 250 | 99 736 | 168 ± 10 | −8 ± 9 | 5.02 ± 0.50 | ||
S19 | Sky brightness | 100 ≤ S < 5000 | 226 242 | 172 ± 10 | −5 ± 9 | 5.24 ± 0.53 | ||
S19 | Sky brightness | 150 ≤ S < 5000 | 160 133 | 173 ± 10 | −6 ± 9 | 5.39 ± 0.57 | ||
S19 | Sky brightness | 200 ≤ S < 5000 | 122 549 | 174 ± 11 | −6 ± 10 | 5.43 ± 0.60 | ||
S19 | Sky brightness | 250 ≤ S < 5000 | 98 205 | 174 ± 11 | −8 ± 10 | 5.64 ± 0.64 |
References. B18: Bengaly et al. (2018); S19: Singal (2019).
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