Behind the Mask: can HARMONI@ELT detect biosignatures in the reflected light of Proxima b?
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| Autores principales: | , , , , , , , , , |
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| Formato: | Preprint |
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2024
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| _version_ | 1866909076238106624 |
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| author | Vaughan, Sophia R. Birkby, Jayne L. Thatte, Niranjan Carlotti, Alexis Houllé, Mathis Pereira-Santaella, Miguel Clarke, Fraser Vigan, Arthur Lin, Zifan Kaltenegger, Lisa |
| author_facet | Vaughan, Sophia R. Birkby, Jayne L. Thatte, Niranjan Carlotti, Alexis Houllé, Mathis Pereira-Santaella, Miguel Clarke, Fraser Vigan, Arthur Lin, Zifan Kaltenegger, Lisa |
| contents | Proxima b is a rocky exoplanet in the habitable zone of the nearest star system and a key test case in the search for extraterrestrial life. Here, we investigate the characterization of a potential Earth-like atmosphere around Proxima b in reflected light via molecule mapping, combining high resolution spectroscopy (HRS) and high contrast imaging, using the first-generation integral field spectrograph HARMONI on the $39$-m Extremely Large Telescope. We simulate comprehensive observations of Proxima b at an assumed $45^{\circ}$ inclination using HARMONI's High Contrast Adaptive Optics mode, with spatial resolution $\sim 8$mas ($3.88$mas/spaxel) and spectral resolving power $R\simeq17,000$ between $1.538$--$1.678 μm$, containing the spectral features of water, carbon dioxide and methane. Tellurics, stellar features, and additional noise sources are included, and removed using established molecule mapping techniques. We find that HARMONI's current focal plane mask (FPM) is too large and obscures the orbit of Proxima b and thus explore smaller and offset FPMs to yield a detection. A $\rm{S/N}=5$ detection of Proxima b's reflected light, suitable for atmospheric characterisation, is possible with such modifications, requiring a minimum of $20$ hours, but ideally at least $30$ hours of integration time. We highlight that such detections do not scale with the photon noise, hence suitably detailed simulations of future instruments for the ELTs are needed to fully understand their ability to perform HRS observations of exoplanet atmospheres. Alterations to the HARMONI FPM design are feasible at this stage, but must be considered in context of other science cases. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2401_09589 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Behind the Mask: can HARMONI@ELT detect biosignatures in the reflected light of Proxima b? Vaughan, Sophia R. Birkby, Jayne L. Thatte, Niranjan Carlotti, Alexis Houllé, Mathis Pereira-Santaella, Miguel Clarke, Fraser Vigan, Arthur Lin, Zifan Kaltenegger, Lisa Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics Proxima b is a rocky exoplanet in the habitable zone of the nearest star system and a key test case in the search for extraterrestrial life. Here, we investigate the characterization of a potential Earth-like atmosphere around Proxima b in reflected light via molecule mapping, combining high resolution spectroscopy (HRS) and high contrast imaging, using the first-generation integral field spectrograph HARMONI on the $39$-m Extremely Large Telescope. We simulate comprehensive observations of Proxima b at an assumed $45^{\circ}$ inclination using HARMONI's High Contrast Adaptive Optics mode, with spatial resolution $\sim 8$mas ($3.88$mas/spaxel) and spectral resolving power $R\simeq17,000$ between $1.538$--$1.678 μm$, containing the spectral features of water, carbon dioxide and methane. Tellurics, stellar features, and additional noise sources are included, and removed using established molecule mapping techniques. We find that HARMONI's current focal plane mask (FPM) is too large and obscures the orbit of Proxima b and thus explore smaller and offset FPMs to yield a detection. A $\rm{S/N}=5$ detection of Proxima b's reflected light, suitable for atmospheric characterisation, is possible with such modifications, requiring a minimum of $20$ hours, but ideally at least $30$ hours of integration time. We highlight that such detections do not scale with the photon noise, hence suitably detailed simulations of future instruments for the ELTs are needed to fully understand their ability to perform HRS observations of exoplanet atmospheres. Alterations to the HARMONI FPM design are feasible at this stage, but must be considered in context of other science cases. |
| title | Behind the Mask: can HARMONI@ELT detect biosignatures in the reflected light of Proxima b? |
| topic | Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2401.09589 |