Learning to See: Applying Inverse Recurrent Inference Machines to See through Refractive Scattering
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arXiv
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| Autori principali: | , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| _version_ | 1866910811757215744 |
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| author | Kouroshnia, Arvin Nguyen, Kenny Ni, Chunchong SaraerToosi, Ali Broderick, Avery E. |
| author_facet | Kouroshnia, Arvin Nguyen, Kenny Ni, Chunchong SaraerToosi, Ali Broderick, Avery E. |
| contents | The Event Horizon Telescope (EHT) has produced horizon-resolving images of Sagittarius A* (Sgr A$^*$). Scattering in the turbulent plasma of the interstellar medium distorts the appearance of Sgr A$^*$ on scales only marginally smaller than the fiducial resolution of EHT. Therefore, this process both diffractive blurs and adds stochastic refractive substructures that limits the practical angular resolution of EHT images of Sgr A$^*$. We utilized a novel recurrent neural network machine learning framework to demonstrate that it is possible to mitigate interstellar scattering at wavelengths of $1.3\,{\rm mm}$ near the galactic center up to structures at the scale of $5μ{as}$ well below the nominal instrumental resolution of EHT, $24\,μ{\rm as}$. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_14055 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Learning to See: Applying Inverse Recurrent Inference Machines to See through Refractive Scattering Kouroshnia, Arvin Nguyen, Kenny Ni, Chunchong SaraerToosi, Ali Broderick, Avery E. Instrumentation and Methods for Astrophysics Astrophysics of Galaxies The Event Horizon Telescope (EHT) has produced horizon-resolving images of Sagittarius A* (Sgr A$^*$). Scattering in the turbulent plasma of the interstellar medium distorts the appearance of Sgr A$^*$ on scales only marginally smaller than the fiducial resolution of EHT. Therefore, this process both diffractive blurs and adds stochastic refractive substructures that limits the practical angular resolution of EHT images of Sgr A$^*$. We utilized a novel recurrent neural network machine learning framework to demonstrate that it is possible to mitigate interstellar scattering at wavelengths of $1.3\,{\rm mm}$ near the galactic center up to structures at the scale of $5μ{as}$ well below the nominal instrumental resolution of EHT, $24\,μ{\rm as}$. |
| title | Learning to See: Applying Inverse Recurrent Inference Machines to See through Refractive Scattering |
| topic | Instrumentation and Methods for Astrophysics Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2501.14055 |