| Article | |
| Report number | arXiv:2211.16547 ; FERMILAB-CONF-22-918-PPD |
| Title | The Second Radio Synchrotron Background Workshop: Conference Summary and Report |
| Author(s) | Singal, J. (Richmond U.) ; Fornengo, N. (INFN, Turin) ; Regis, M. (INFN, Turin) ; Bernardi, G. (Bologna, Ist. Radioastronomia ; Rhodes U. ; South African Astron. Observ.) ; Bordenave, D. (Virginia U., Astron. Dept. ; NRAO, Charlottesville) ; Branchini, E. (Rome III U. ; Genoa U. ; INFN, Genoa) ; Cappelluti, N. (Miami U.) ; Caputo, A. (Tel Aviv U. ; Weizmann Inst. ; CERN) ; Carucci, I.P. (INFN, Turin) ; Chluba, J. (Jodrell Bank ; U. Manchester (main)) ; Cuoco, A. (INFN, Turin) ; DiLullo, C. (NASA, Goddard) ; Fialkov, A. (Cambridge U.) ; Hale, C. (Edinburgh U., Inst. Astron.) ; Harper, S.E. (Jodrell Bank ; U. Manchester (main)) ; Heston, S. (Virginia Tech., Blacksburg) ; Holder, G. (Illinois U., Urbana) ; Kogut, A. (NASA, Goddard) ; Krause, M.G. H. (Hertfordshire U.) ; Leahy, J.P. (Jodrell Bank ; U. Manchester (main)) ; Mittal, S. (Tata Inst.) ; Monsalve, R.A. (UC, Berkeley (main) ; Arizona State U. ; Concepcion Catolica U.) ; Piccirilli, G. (Rome U., Tor Vergata) ; Pinetti, E. (Fermilab ; Chicago U., Astron. Astrophys. Ctr. ; Chicago U., EFI ; Chicago U., KICP) ; Recchia, S. (INFN, Turin) ; Taoso, M. (INFN, Turin) ; Todarello, E. (INFN, Turin) |
| Publication | 2023-03-20 |
| Imprint | 2022-11-29 |
| Number of pages | 33 |
| Note | 34 pages, 19 figures, 3 tables, accepted to PASP, updated to in press version |
| In: | Publ. Astron. Soc. Pac. |
| In: | 2nd Radio Synchrotron Background Conference, Barolo, Italy, 14 - 18 Jun 2022, pp.036001 |
| DOI | 10.1088/1538-3873/acbdbf |
| Subject category | astro-ph.CO ; Astrophysics and Astronomy |
| Abstract | We summarize the second radio synchrotron background workshop, which took place June 15-17, 2022 in Barolo, Italy. This meeting was convened because available measurements of the diffuse radio zero level continue to suggest that it is several times higher than can be attributed to known Galactic and extragalactic sources and processes, rendering it the least well understood electromagnetic background at present and a major outstanding question in astrophysics. The workshop agreed on the next priorities for investigations of this phenomenon, which include searching for evidence of the Radio Sunyaev-Zel'dovich effect, carrying out cross-correlation analyses of radio emission with other tracers, and supporting the completion of the 310 MHz absolutely calibrated sky map project. |
| Copyright/License | preprint: (License: arXiv nonexclusive-distrib 1.0) publication: © 2023-2024 The Author(s) (License: CC-BY-3.0) |
Corresponding record in: Inspire
Record created 2022-12-10, last modified 2024-12-18