A dataset provided by the European Space Agency

Name: Looking for the mCP Rosetta Stone - A Comparative Survey of Magnetospheres
Published: 2011-11-04T00:00:00Z

Proposal ID	065522
Title	Looking for the mCP Rosetta Stone - A Comparative Survey of Magnetospheres
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655220201
DOI	https://doi.org/10.5270/esa-angxi8d
Principal Investigator, PI	Dr Vito Graffagnino
Abstract	We propose to obtain EPIC spectra and lightcurves of a sample of 8 youngmagnetic early type stars, four of which were previously detected as X-raysources by ROSAT, and all of which are known to be characterised as non-thermalradio sources. An additional two sources will be used as control subjects sincethese are known to be older A-type stars. Together, this sample provides a rangeof B fields, rotation periods, age and radio fluxes that allow will help us torelate the detected X-ray flux and/or spectrum to the underlying physicalproperties of the confined magnetospheric plasma.
Publications	X-rays from magnetic intermediate mass Ap/Bp stars \|Robrade Jan \| AdSpR \| 58-727 \| 2016 \| 2016AdSpR..58..727R \| http://ui.adsabs.harvard.edu/#abs/2016AdSpR..58..727R 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 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	2010-10-06T04:00:04Z/2010-10-06T09:55:22Z
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	2011-11-04T00:00:00Z
Last Update	2025-01-27
Keywords	"additional sources", "nonthermal radio sources", "EPIC", "epic spectra", "radio fluxes", "type stars", "rotation periods", "xray flux", "ROSAT", "xray sources", "physical properties", "comparative survey", "mcp rosetta stone", "control subjects", "confined magnetospheric plasma"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Vito Graffagnino, 2011, 'Looking for the mCP Rosetta Stone - A Comparative Survey of Magnetospheres', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-angxi8d