A dataset provided by the European Space Agency

Name: The X-ray irradiation of transiting extra-solar planets
Published: 2007-12-08T00:00:00Z

Proposal ID	040445
Title	The X-ray irradiation of transiting extra-solar planets
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0404450101
DOI	https://doi.org/10.5270/esa-qe1hddq
Principal Investigator, PI	Dr Peter Wheatley
Abstract	The evolution and observed properties of close-in extra-solar planets may becontrolled by X-ray irradiation by their parent stars. Transiting planetsprovide a unique opportunity to study the effect of irradiation on mass lossfrom close-in planets and the possible consequent effects on their mass-radiusrelation. To date, however, theoretical studies have relied on estimates of theirradiating flux in each system. Here we propose to observe the four brighttransiting planets with XMM-Newton in order to measure the irradiating flux. Inparticular we intend to test the suggestion that HD209458b is losing mass due toX-ray irradiation-driven evaporation.
Publications	Estimation of the XUV radiation onto close planets and their evaporation \|Sanz-Forcada, J., Micela, G., et al. \| A&A \| 532-6 \| 2011 \| 2011A&A...532A...6S \| http://ui.adsabs.harvard.edu/#abs/2011A&A...532A...6S A scenario of planet erosion by coronal radiation \|Sanz-Forcada, J., Ribas, I., et al. \| A&A \| 511-8 \| 2010 \| 2010A&A...511L...8S \| http://ui.adsabs.harvard.edu/#abs/2010A&A...511L...8S An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti, F., Middei, R., et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 Reconstructing the high-energy irradiation of the evaporating hot Jupiter HD 209458b \|Louden, Tom, Wheatley, Peter J., \| MNRAS \| 464-2396 \| 2017 \| 2017MNRAS.464.2396L \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.464.2396L A scenario of planet erosion by coronal radiation (Corrigendum) \|Sanz-Forcada, J., Ribas, I., et al. \| A&A \| 520-1 \| 2010 \| 2010A&A...520C...1S \| http://ui.adsabs.harvard.edu/#abs/2010A&A...520C...1S Coronal X-ray emission and planetary irradiation in HD 209458 \|Czesla, S., Salz, M., et al. \| A&A \| 607-101 \| 2017 \| 2017A&A...607A.101C \| http://ui.adsabs.harvard.edu/#abs/2017A&A...607A.101C 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 X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C The Relative Emission from Chromospheres and Coronae: Dependence on Spectral Type and Age \|Linsky, Jeffrey L., Wood, Brian E., et al. \| ApJ \| 902-3 \| 2020 \| 2020ApJ...902....3L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...902....3L An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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 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	2006-11-14T23:49:21Z/2006-11-15T09:07:56Z
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	2007-12-08T00:00:00Z
Keywords	"parent stars", "XMM", "irradiating flux", "transiting planets", "HD209458", "losing mass", "bright transiting planets", "mass loss", "XMM-Newton", "mass radius relation", "xray irradiation", "consequent effects", "extra solar planets", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Peter Wheatley, 2007, 'The X-ray irradiation of transiting extra-solar planets', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qe1hddq