A dataset provided by the European Space Agency

Name 087180
Title Essential Ultraviolet Stellar Characterization for Guaranteed JWST Transiting Pl
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0871800101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0871800201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0871800301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0871800401

DOI https://doi.org/10.57780/esa-nwt2m8i
Author Dr Kevin France
Description JWST will launch during HST cycle 28 and begin a new era in atmospheric
characterization for all types of exoplanets. Atmospheric spectroscopy of warm
rocky planets, sub-Neptune, and Jupiter-mass planets will be obtained through a
robust set of guaranteed transiting planet observations (the JWST ERS and GTO
programs). We propose to obtain temporally-resolved UV (1150-3200 Ang) stellar
spectroscopy of the 13 JWST guaranteed time targets with no UV characterization
data in the HST archive. Our proposed observations will provide the UV context
necessary to determine the likelihood of atmospheric formation and retention,
the identification and interpretation of atmospheric chemistry, and the impacts
of stellar activity on the exoplanet atmospheric stability.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2021-04-15T07:42:55Z/2021-05-15T14:07:07Z
Version PPS_NOT_AVAILABLE
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2022-06-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Kevin France, 2022, 087180, PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.57780/esa-nwt2m8i