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
Last Update	2025-01-27
Keywords	"photometric variations", "orbital periods", "xmm newton", "XMM-Newton", "xray luminosities", "transiting systems", "suitable objects", "XMM", "hydrodynamic blow", "xray survey", "energy properties", "prime candidates", "ca ii emission", "planetary atmospheric evaporation"
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