Bolometric interferometry and spectral: a QUBIC overview
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arXiv
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| Format: | Preprint |
| Veröffentlicht: |
2024
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| _version_ | 1866916313178308608 |
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| author | Laclavère, Tom |
| author_facet | Laclavère, Tom |
| contents | The Q \& U Bolometric Interferometer for Cosmology (QUBIC) is a new kind of cosmological instrument that uses interferometry to observe the sky. The unique synthesized beam of QUBIC has an important frequency dépendance that we use to increase spectral resolution and perform new component separation methods, allowing us to mitigate foreground contamination in an improved manner. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_15414 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Bolometric interferometry and spectral: a QUBIC overview Laclavère, Tom Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics The Q \& U Bolometric Interferometer for Cosmology (QUBIC) is a new kind of cosmological instrument that uses interferometry to observe the sky. The unique synthesized beam of QUBIC has an important frequency dépendance that we use to increase spectral resolution and perform new component separation methods, allowing us to mitigate foreground contamination in an improved manner. |
| title | Bolometric interferometry and spectral: a QUBIC overview |
| topic | Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2406.15414 |