A dataset provided by the European Space Agency

Name: An X-ray survey of ultra-active planet hosts
Published: 2015-11-04T23:00:00Z

Proposal ID	074346
Title	An X-ray survey of ultra-active planet hosts
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743460101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743460201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743460301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743460501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743460701
DOI	https://doi.org/10.5270/esa-wd35q25
Principal Investigator, PI	Prof Jurgen Schmitt
Abstract	We propose to obtain snapshot observations of a sample of ultra-active planethosts. The sample is complete in that it comprises all known transiting systems(not observed/proposed) within 250 pc, orbital periods below 10 days and strongactivity as photometric variations in excess of 1% and/or Ca II emission; thesample does include all suitable objects detected by Kepler. The sensitivity ofthe proposed XMM-Newton observations allows the detection of stars with X-rayluminosities in excess of 10^29 erg/sec. Because of the proximity to their hoststhese planets are the prime candidates for the process of planetary atmosphericevaporation through hydrodynamic blow-off. With our study we establish thehosts high-energy properties and pave the way for meaningful follow-up studies.
Publications	Differences in the fast optical variability of the dwarf nova V1504 Cyg between quiescence and outbursts detected in Kepler data and simulations of the rms-flux relations \|Dobrotka A. Ness J.-U. \| MNRAS \| 451-2851 \| 2015 \| 2015MNRAS.451.2851D \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.451.2851D The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F An improved age-activity relationship for cool stars older than a gigayear \|Booth R. S. Poppenhaeger K. et al. \| MNRAS \| 471-1012 \| 2017 \| 2017MNRAS.471.1012B \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1012B Atmospheric mass-loss of extrasolar planets orbiting magnetically active host stars \|Lalitha Sairam Schmitt J. H. M. M. \| MNRAS \| 477-808 \| 2018 \| 2018MNRAS.477..808L \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.477..808L 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 X-ray activity of the young solar-like star Kepler-63 and the structure of its corona \|Coffaro M. Stelzer B. \| A&A \| 661-79 \| 2022 \| 2022A&A...661A..79C \| http://ui.adsabs.harvard.edu/#abs/2022A&A...661A..79C Characterizing X-ray activity cycles of young solar-like stars with solar observations \|Coffaro Martina Stelzer Beate \| AN \| 343-10066 \| 2022 \| 2022AN....34310066C \| http://ui.adsabs.harvard.edu/#abs/2022AN....34310066C XMM-Newton observation of V1504 Cyg as a probe for the existence of an evaporated corona \|Dobrotka A. Ness J. -U. et al. \| A&A \| 674-188 \| 2023 \| 2023A&A...674A.188D \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A.188D 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	2014-07-10T12:21:46Z/2014-10-22T00:54:23Z
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	2015-11-04T23:00:00Z
Keywords	"suitable objects", "prime candidates", "photometric variations", "XMM", "planetary atmospheric evaporation", "xmm newton", "transiting systems", "energy properties", "hydrodynamic blow", "xray survey", "XMM-Newton", "orbital periods", "ca ii emission", "xray luminosities"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Jurgen Schmitt, 2015, 'An X-ray survey of ultra-active planet hosts', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-wd35q25