A dataset provided by the European Space Agency

Name 060558
Title Planet Induced Stellar Activity: an X-ray Optical Study of 2 Contrasting Systems
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605580201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605580301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605580401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605580501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605580601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605580701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605580801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605580901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605581001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605581101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605581201
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605581301
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605581501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605581601

DOI https://doi.org/10.5270/esa-rrp4tpe
Author Dr Stefan Dieters
Description For 2 contrasting systems we plan to investigate the influence the Hot Jupiters have upon their host stars using phase (planetary orbital and stellar rotational) resolved spectroscopy. By combining our X-ray and UV data with contemporaneous optical spectropolarimetric observations we will be able to test and enhance current models for the magnetic interaction between stars and their giant close-in planets.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-09-21T21:07:43Z/2009-10-27T23:38:24Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2010-12-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-12-09T00:00:00Z, 060558, 17.56_20190403_1200. https://doi.org/10.5270/esa-rrp4tpe