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| Auteurs principaux: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
| Publié: |
2024
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| Sujets: | |
| Accès en ligne: | https://arxiv.org/abs/2406.01492 |
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| _version_ | 1866910469700190208 |
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| author | Soares-Furtado, Melinda Limbach, Mary Anne Vanderburg, Andrew Bally, John Becker, Juliette Rosen, Anna L. Bouma, Luke G. Vos, Johanna M. Howell, Steve B. Beatty, Thomas G. Best, William M. J. Cody, Anne Marie Distler, Adam D'Onghia, Elena Heller, René Hensley, Brandon S. Hinkel, Natalie R. Jackson, Brian Kounkel, Marina Kraus, Adam Mann, Andrew W. Marston, Nicholas T. Robberto, Massimo Rodriguez, Joseph E. Steffen, Jason H. Teske, Johanna K. Townsend, Richard Yarza, Ricardo Youngblood, Allison |
| author_facet | Soares-Furtado, Melinda Limbach, Mary Anne Vanderburg, Andrew Bally, John Becker, Juliette Rosen, Anna L. Bouma, Luke G. Vos, Johanna M. Howell, Steve B. Beatty, Thomas G. Best, William M. J. Cody, Anne Marie Distler, Adam D'Onghia, Elena Heller, René Hensley, Brandon S. Hinkel, Natalie R. Jackson, Brian Kounkel, Marina Kraus, Adam Mann, Andrew W. Marston, Nicholas T. Robberto, Massimo Rodriguez, Joseph E. Steffen, Jason H. Teske, Johanna K. Townsend, Richard Yarza, Ricardo Youngblood, Allison |
| contents | The TEMPO (Transiting Exosatellites, Moons, and Planets in Orion) Survey is a proposed 30-day observational campaign using the Nancy Grace Roman Space Telescope. By providing deep, high-resolution, short-cadence infrared photometry of a dynamic star-forming region, TEMPO will investigate the demographics of exosatellites orbiting free-floating planets and brown dwarfs -- a largely unexplored discovery space. Here, we present the simulated detection yields of three populations: extrasolar moon analogs orbiting free-floating planets, exosatellites orbiting brown dwarfs, and exoplanets orbiting young stars. Additionally, we outline a comprehensive range of anticipated scientific outcomes accompanying such a survey. These science drivers include: obtaining observational constraints to test prevailing theories of moon, planet, and star formation; directly detecting widely separated exoplanets orbiting young stars; investigating the variability of young stars and brown dwarfs; constraining the low-mass end of the stellar initial mass function; constructing the distribution of dust in the Orion Nebula and mapping evolution in the near-infrared extinction law; mapping emission features that trace the shocked gas in the region; constructing a dynamical map of Orion members using proper motions; and searching for extragalactic sources and transients via deep extragalactic observations reaching a limiting magnitude of $m_{AB}=29.7$\,mag (F146 filter). |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_01492 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The TEMPO Survey II: Science Cases Leveraged from a Proposed 30-Day Time Domain Survey of the Orion Nebula with the Nancy Grace Roman Space Telescope Soares-Furtado, Melinda Limbach, Mary Anne Vanderburg, Andrew Bally, John Becker, Juliette Rosen, Anna L. Bouma, Luke G. Vos, Johanna M. Howell, Steve B. Beatty, Thomas G. Best, William M. J. Cody, Anne Marie Distler, Adam D'Onghia, Elena Heller, René Hensley, Brandon S. Hinkel, Natalie R. Jackson, Brian Kounkel, Marina Kraus, Adam Mann, Andrew W. Marston, Nicholas T. Robberto, Massimo Rodriguez, Joseph E. Steffen, Jason H. Teske, Johanna K. Townsend, Richard Yarza, Ricardo Youngblood, Allison Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics The TEMPO (Transiting Exosatellites, Moons, and Planets in Orion) Survey is a proposed 30-day observational campaign using the Nancy Grace Roman Space Telescope. By providing deep, high-resolution, short-cadence infrared photometry of a dynamic star-forming region, TEMPO will investigate the demographics of exosatellites orbiting free-floating planets and brown dwarfs -- a largely unexplored discovery space. Here, we present the simulated detection yields of three populations: extrasolar moon analogs orbiting free-floating planets, exosatellites orbiting brown dwarfs, and exoplanets orbiting young stars. Additionally, we outline a comprehensive range of anticipated scientific outcomes accompanying such a survey. These science drivers include: obtaining observational constraints to test prevailing theories of moon, planet, and star formation; directly detecting widely separated exoplanets orbiting young stars; investigating the variability of young stars and brown dwarfs; constraining the low-mass end of the stellar initial mass function; constructing the distribution of dust in the Orion Nebula and mapping evolution in the near-infrared extinction law; mapping emission features that trace the shocked gas in the region; constructing a dynamical map of Orion members using proper motions; and searching for extragalactic sources and transients via deep extragalactic observations reaching a limiting magnitude of $m_{AB}=29.7$\,mag (F146 filter). |
| title | The TEMPO Survey II: Science Cases Leveraged from a Proposed 30-Day Time Domain Survey of the Orion Nebula with the Nancy Grace Roman Space Telescope |
| topic | Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2406.01492 |