The Dragonfly Spectral Line Mapper: Completion of the 120-lens array
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arXiv
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| Auteurs principaux: | , , , , , , , , , |
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| Format: | Preprint |
| Publié: |
2024
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| _version_ | 1866909228912869376 |
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| author | Chen, Seery Lokhorst, Deborah M. Pasha, Imad Bowman, William P. Liu, Qing Shen, Zili MacNichol, Aidan Malakhov, Evgeni I. Abraham, Roberto G. van Dokkum, Pieter |
| author_facet | Chen, Seery Lokhorst, Deborah M. Pasha, Imad Bowman, William P. Liu, Qing Shen, Zili MacNichol, Aidan Malakhov, Evgeni I. Abraham, Roberto G. van Dokkum, Pieter |
| contents | The Dragonfly Spectral Line Mapper is a mosaic telescope comprising 120 Canon telephoto lenses, based on the design of the Dragonfly Telephoto Array. With a wide field of view, and the addition of the "Dragonfly Filter-Tilter" instrumentation holding ultra narrow bandpass filters in front of each lens, the Dragonfly Spectral Line mapper is optimized for ultra low surface brightness imaging of visible wavelength line emission. The Dragonfly Spectral Line Mapper was constructed and commissioned in four phases from March 2022 to November 2023. During this time, four individual mounts of 30 lenses each were constructed and commissioned. The commissioning of the telescope included the deployment of the "Dragonfly StarChaser" which carries out image stabilization corrections in the telephoto lens, to enable hour-long exposures to be taken. In addition, we introduced new instrumentation such as a film to cover the optics to keep the filters clean. Here we describe the updated design of the complete 120-lens array, and the implementation of the instrumentation described above. Additionally, we present updated characterization of the cameras and filter transmission for the full array. Finally, we reflect on the construction and commissioning process of the complete 120-lens array Dragonfly Spectral Line Mapper, and remark on the feasibility of a larger 1000-lens array. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_15101 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The Dragonfly Spectral Line Mapper: Completion of the 120-lens array Chen, Seery Lokhorst, Deborah M. Pasha, Imad Bowman, William P. Liu, Qing Shen, Zili MacNichol, Aidan Malakhov, Evgeni I. Abraham, Roberto G. van Dokkum, Pieter Instrumentation and Methods for Astrophysics The Dragonfly Spectral Line Mapper is a mosaic telescope comprising 120 Canon telephoto lenses, based on the design of the Dragonfly Telephoto Array. With a wide field of view, and the addition of the "Dragonfly Filter-Tilter" instrumentation holding ultra narrow bandpass filters in front of each lens, the Dragonfly Spectral Line mapper is optimized for ultra low surface brightness imaging of visible wavelength line emission. The Dragonfly Spectral Line Mapper was constructed and commissioned in four phases from March 2022 to November 2023. During this time, four individual mounts of 30 lenses each were constructed and commissioned. The commissioning of the telescope included the deployment of the "Dragonfly StarChaser" which carries out image stabilization corrections in the telephoto lens, to enable hour-long exposures to be taken. In addition, we introduced new instrumentation such as a film to cover the optics to keep the filters clean. Here we describe the updated design of the complete 120-lens array, and the implementation of the instrumentation described above. Additionally, we present updated characterization of the cameras and filter transmission for the full array. Finally, we reflect on the construction and commissioning process of the complete 120-lens array Dragonfly Spectral Line Mapper, and remark on the feasibility of a larger 1000-lens array. |
| title | The Dragonfly Spectral Line Mapper: Completion of the 120-lens array |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2406.15101 |