The Roman coronagraph community participation program: observation planning
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arXiv
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| Auteurs principaux: | , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Publié: |
2024
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| _version_ | 1866912134287327232 |
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| author | Wolff, Schuyler G. Wang, Jason Stapelfeldt, Karl Bailey, Vanessa P. Savransky, Dmitry Hom, Justin Biller, Beth Brandner, Wolfgang Anche, Ramye Blunt, Sarah Brinjikji, Marah Girard, Julien H. Krause, Oliver Li, Zhexing Livingston, John Millar-Blanchaer, Maxwell A. Noel, Malachi Pueyo, Laurent De Rosa, Robert J. Samland, Matthias Schragal, Nicholas |
| author_facet | Wolff, Schuyler G. Wang, Jason Stapelfeldt, Karl Bailey, Vanessa P. Savransky, Dmitry Hom, Justin Biller, Beth Brandner, Wolfgang Anche, Ramye Blunt, Sarah Brinjikji, Marah Girard, Julien H. Krause, Oliver Li, Zhexing Livingston, John Millar-Blanchaer, Maxwell A. Noel, Malachi Pueyo, Laurent De Rosa, Robert J. Samland, Matthias Schragal, Nicholas |
| contents | The Coronagraphic Instrument onboard the Nancy Grace Roman Space Telescope is an important stepping stone towards the characterization of habitable, rocky exoplanets. In a technology demonstration phase conducted during the first 18 months of the mission (expected to launch in late 2026), novel starlight suppression technology may enable direct imaging of a Jupiter analog in reflected light. Here we summarize the current activities of the Observation Planning working group formed as part of the Community Participation Program. This working group is responsible for target selection and observation planning of both science and calibration targets in the technology demonstration phase of the Roman Coronagraph. We will discuss the ongoing efforts to expand target and reference catalogs, and to model astrophysical targets (exoplanets and circumstellar disks) within the Coronagraph's expected sensitivity. We will also present preparatory observations of high priority targets. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2411_17868 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The Roman coronagraph community participation program: observation planning Wolff, Schuyler G. Wang, Jason Stapelfeldt, Karl Bailey, Vanessa P. Savransky, Dmitry Hom, Justin Biller, Beth Brandner, Wolfgang Anche, Ramye Blunt, Sarah Brinjikji, Marah Girard, Julien H. Krause, Oliver Li, Zhexing Livingston, John Millar-Blanchaer, Maxwell A. Noel, Malachi Pueyo, Laurent De Rosa, Robert J. Samland, Matthias Schragal, Nicholas Instrumentation and Methods for Astrophysics The Coronagraphic Instrument onboard the Nancy Grace Roman Space Telescope is an important stepping stone towards the characterization of habitable, rocky exoplanets. In a technology demonstration phase conducted during the first 18 months of the mission (expected to launch in late 2026), novel starlight suppression technology may enable direct imaging of a Jupiter analog in reflected light. Here we summarize the current activities of the Observation Planning working group formed as part of the Community Participation Program. This working group is responsible for target selection and observation planning of both science and calibration targets in the technology demonstration phase of the Roman Coronagraph. We will discuss the ongoing efforts to expand target and reference catalogs, and to model astrophysical targets (exoplanets and circumstellar disks) within the Coronagraph's expected sensitivity. We will also present preparatory observations of high priority targets. |
| title | The Roman coronagraph community participation program: observation planning |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2411.17868 |