A dataset provided by the European Space Agency

Name: High energy irradiation and mass loss on the super earth GJ 1214b
Published: 2014-10-10T00:00:00Z

Proposal ID	072438
Title	High energy irradiation and mass loss on the super earth GJ 1214b
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724380101
DOI	https://doi.org/10.5270/esa-jt8jafn
Principal Investigator, PI	Ms Lalitha Sairam
Abstract	We propose to observe the transiting super-earth system GJ 1214 for 25 ks withXMM-Newton. GJ 1214 is located 13 pc from Earth and shows the deepestvisual-band transit of all close super-earths. The system is a suitable targetfor observations and, thus, a test-case for planetary and atmospheric modeling.The proposed observation will allow us to characterize the X-ray and UV emissionof the host star, estimate the mass-loss rate and history of the planet,constrain models of GJ 1214b s atmosphere, and, finally, prepare the ground formore intensive follow-up studies.
Publications	X-Ray Emission from the Super-Earth Host GJ 1214 \|Lalitha S. Poppenhaeger K. et al. \| ApJ \| 790-11 \| 2014 \| 2014ApJ...790L..11L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...790L..11L The MUSCLES Treasury Survey. I. Motivation and Overview \|France Kevin Parke Loyd R. O. et al. \| ApJ \| 820-89 \| 2016 \| 2016ApJ...820...89F \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...820...89F 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 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 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 A tentative detection of He I in the atmosphere of GJ 1214 b \|Orell-Miquel J. Murgas F. et al. \| A&A \| 659-55 \| 2022 \| 2022A&A...659A..55O \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..55O 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-09-27T17:50:14Z/2013-09-28T03:45:14Z
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	2014-10-10T00:00:00Z
Last Update	2025-01-27
Keywords	"suitable target", "mass loss", "gj 1214b", "xmm newton", "gj 1214", "close super earths", "constrain models", "XMM-Newton", "atmospheric modeling", "uv emission", "XMM", "mass loss rate", "energy irradiation"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Ms Lalitha Sairam, 2014, 'High energy irradiation and mass loss on the super earth GJ 1214b', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jt8jafn