Details on Acronym: [VSP2022] | |
| [VSP2022] | (Vacca+Shimwell+Perley+, 2022) |
| Write: | <<[VSP2022] SNN>> <<[VSP2022] FN>> <<[VSP2022] P>> |
| N: | 10+3+1 |
| Object: | (Rad) (SIMBAD class: Radio = Radio Source) |
| Note: | LOFAR 144MHz and VLA 1.410 and 1.782GHz observations of N=10 sources, N=3 filaments, and N=1 "roundish patch of emission" in Abell 523. |
| in source: | ACO 523 |
| Ref: | =2022MNRAS.511.3389V |
| by | VACCA V. , SHIMWELL T., PERLEY R.A., GOVONI F., MURGIA M., FERETTI L., GIOVANNINI G., LOI F., CARRETTI E., COVA F., GASTALDELLO F., GIRARDI M., ENSSLIN T., AKAMATSU H., BONAFEDE A., BONNASSIEUX E., BOSCHIN W., BOTTEON A., BRUNETTI G., BRUGGEN M., FINOGUENOV A., HOANG D., IACOBELLI M., ORRU E., PALADINO R., ROTTGERING H., VAN WEEREN R., VITELLO F., WITTOR D. |
| Mon. Not. R. Astron. Soc., 511, 3389-3407 (2022) | |
| Spectral study of the diffuse synchrotron source in the galaxy cluster Abell 523. | |
| o | Figs 1-2, Table 3: <[VSP2022] SNN> (Nos S1-S10), <[VSP2022] FN> (Nos F1-F3), <[VSP2022] P> N=1. |
| Origin | of the Acronym: D = Assigned by the Dictionary of Acronyms |