A dataset provided by the European Space Agency

Name: High-energy irradiation of WASP-69 b: powering an extreme planetary wind
Published: 2017-11-11T23:00:00Z

Proposal ID	078356
Title	High-energy irradiation of WASP-69 b: powering an extreme planetary wind
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783560201
DOI	https://doi.org/10.5270/esa-5wlg88m
Principal Investigator, PI	Mr Michael Salz
Abstract	Stellar X-ray irradiation drives planetary winds, whose properties remainlargely unknown. WASP-69 b could be the most heavily evaporating hot Neptunewithin 100 pc, driving a wind 50 times stronger than that of HD 189733 b. Thismakes the system a highly promising new target for transit studies. The X-rayproperties of the host star remain puzzling, however. Scaling the Ca H&Kemission suggests an X-ray luminosity of 1-6e28 erg/s -- consistent with itsprevious identification with a ROSAT source at 60 distance. However, in afollow-up SWIFT snapshot, neither X-ray emission from WASP-69 nor the ROSATsource were detected. We propose a dedicated XMM observation to quantify theX-ray properties of WASP-69 and study the strong planetary wind.
Publications	Ground-based detection of an extended helium atmosphere in the Saturn-mass exoplanet WASP-69b \|Nortmann Lisa Palle Enric et al. \| Sci \| 362-1388 \| 2018 \| 2018Sci...362.1388N \| http://ui.adsabs.harvard.edu/#abs/2018Sci...362.1388N Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Planetary Parameters XUV Environments and Mass-loss Rates for Nearby Gaseous Planets with X-Ray-detected Host Stars \|Spinelli Riccardo Gallo Elena et al. \| AJ \| 165-200 \| 2023 \| 2023AJ....165..200S \| http://ui.adsabs.harvard.edu/#abs/2023AJ....165..200S The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M Exoplanet Aeronomy: A Case Study of WASP-69 bs Variable Thermosphere \|Levine W. Garrett Vissapragada Shreyas et al. \| AJ \| 168-65 \| 2024 \| 2024AJ....168...65L \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168...65L New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-10-21T04:52:32Z/2016-10-21T13:29:12Z
Version	17.56_20190403_1200
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	2017-11-11T23:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "energy irradiation", "xray luminosity", "rosat source", "swift snapshot", "hd 189733", "HD 189733", "6e28 erg", "ROSAT", "planetary wind", "xray properties", "dedicated xmm", "xray emission"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Michael Salz, 2017, 'High-energy irradiation of WASP-69 b: powering an extreme planetary wind', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5wlg88m