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...
I tiakina i:
| Ngā kaituhi matua: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Maynooth Academic Publishing
2026-07-01
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| Rangatū: | The Open Journal of Astrophysics |
| Urunga tuihono: | https://doi.org/10.33232/001c.165326 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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