Characterization of the Polarization Beam Response of SPT-3G Using Point Sources
Precise measurements of cosmic microwave background (CMB) polarization require rigorous control of instrumental systematics. For the South Pole Telescope's third-generation camera (SPT-3G), which observes in three frequency bands roughly centered on 95, 150, and 220 GHz, accurate characterization of...
Furkejuvvon:
| Váldodahkkit: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
Maynooth Academic Publishing
2026-07-01
|
| Ráidu: | The Open Journal of Astrophysics |
| Liŋkkat: | https://doi.org/10.33232/001c.165326 |
| Fáddágilkorat: |
Eai fáddágilkorat, Lasit vuosttaš fáddágilkora!
|
