A dataset provided by the European Space Agency

Name: Star-Planet Magnetic Interaction in Extra-Solar Systems with Hot Jupiters
Published: 2016-10-16T22:00:00Z

Proposal ID	076370
Title	Star-Planet Magnetic Interaction in Extra-Solar Systems with Hot Jupiters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763700301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763700401
DOI	https://doi.org/10.5270/esa-zseav17
Principal Investigator, PI	Dr Antonio Maggio
Abstract	The significant fraction of Jupiter-size exoplanets orbiting at a few stellarradii from the parent stars (hot Jupiters) rises the question whether effects ofmagnetic star-planet interactions (SPI) can be detected. We focus our attentionon systems with eccentric orbits, where we expect to detect systematic effects,like enhanced stellar activity, when the planet is at the closest separation. Wepropose a follow up campaign in X-rays of the system HD 162020 to confirm aprevious SPI effect suggested by observations with Suzaku. Comparison with modelpredictions will allow us to infer the energy budget involved in SPI and thestrength of the magnetic field of the planet.
Publications	The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters \|Pastor-Marazuela, I., Webb, N. A., et al. \| A&A \| 640-124 \| 2020 \| 2020A&A...640A.124P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...640A.124P 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2015-09-13T19:46:36Z/2015-10-05T06:18:30Z
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	2016-10-16T22:00:00Z
Keywords	"magnetic field", "systematic effects", "extra solar systems", "closest separation", "enhanced stellar activity", "system hd 162020", "HD 162020", "energy budget involved", "spi effect suggested", "stellar radii", "model predictions", "hot jupiters", "eccentric orbits"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Antonio Maggio, 2016, 'Star-Planet Magnetic Interaction in Extra-Solar Systems with Hot Jupiters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zseav17