Table 4
Largest relative deviation max(
) between any two sky models m1 and m2 for each of the selected radio experiments.
| Experiment/observatory | ℓexp (°) | Frequency band (MHz) | max( ) (%) |
Corresponding sky models |
|---|---|---|---|---|
| RNO-G (1) | 72.58 | 100–108 | 17.1 | LFSM/GSM16 |
| LOFAR low (2) | 52.91 | 30–80 | 19.8 | ULSA/GMOSS |
| LOFAR high (3) | 52.91 | 110–190 | 18.4 | LFSM/GSM16 |
| GRAND (4) | 42.93 | 50–200 | 21.5 | LFSM/GMOSS |
| OVRO-LWA (5) | 37.23 | 30–80 | 19.3 | ULSA/GMOSS |
| SKA-low (6) | −26.70 | 50–350 | 15.1 | LFSM/GMOSS |
| Auger (7) | −35.21 | 30–80 | 11.7 | LFSM/GMOSS |
| IceCube (8) | −90.0 | 70–350 | 20.3 | LFSM/GMOSS |
Notes. Site locations and frequency bands of the experiments are quoted from latest design plans. For RNO-G the LPDA surface antennas were considered, which are sensitive up to ~1 GHz, but the comparison was done only up to 408 MHz because of the limitations of the LFmap and LFSM sky models. The complete table can be found in Appendix A.
References. (1) Aguilar et al. (2021); (2) Schellart et al. (2013); (3) Nelles et al. (2015); (4) Álvarez-Mufiiz et al. (2020); (5) Monroe et al. (2020); (6) Buitink et al. (2021); (7) De Jong (2021); (8) Abbasi et al. (2021).
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