| Proposal ID | 089200 |
| Title | Essential Ultraviolet Stellar Characterization for Cycle 1 JWST Transiting Plane |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0892000101 |
| DOI | https://doi.org/10.57780/esa-39bl3hi |
| Principal Investigator, PI | Dr Allison Youngblood |
| Abstract | Atmospheric spectroscopy of an exciting array of exoplanets (warm rocky planets,sub-Neptune, and Jupiter mass planets) will be obtained during JWST.s Cycle 1.To accurately model and interpret observations of these planets. atmospheres, wemust understand the high-energy SED of their host stars: FUV and NUV-drivenphotochemistry shapes an atmosphere.s molecular abundances and the formation ofhazes, EUV irradiation can erode a planet.s gaseous envelope, and flares canaffect long term atmospheric stability. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2021-12-26T15:24:34Z/2023-06-18T23:49:38Z |
| Version | 20.10_20230417_1156 |
| Mission Description | The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis. |
| Creator Contact | https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk |
| Date Published | 2024-07-11T00:00:00Z |
| Keywords | "atmospheric spectroscopy", "molecular abundance", "exciting array", "euv irradiation", "energy sed", "gaseous envelope", "ultraviolet stellar characterization", "sub neptune", "jwst transiting plane", "term atmospheric stability", "jupiter mass planets" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Allison Youngblood, 2024, 'Essential Ultraviolet Stellar Characterization for Cycle 1 JWST Transiting Plane', 20.10_20230417_1156, European Space Agency, https://doi.org/10.57780/esa-39bl3hi |