A dataset provided by the European Space Agency

Proposal ID 030420
Title Extrasolar Giant Planets and Stellar Magnetic Activity
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304200301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304200401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304200501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304200801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304200901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304201001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304201101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304201301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304201401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304201501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304201601
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304201801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304202101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304202201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304202301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304202501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304202601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304202701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304202901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304203201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304203301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0304203401

DOI https://doi.org/10.5270/esa-p9t6qup
Principal Investigator, PI Dr Vinay Kashyap
Abstract In order to explore the effect of a new variable governing the magnetic activityof stars, viz., the presence of giant planets, we propose a set of snapshotobservations of a carefully selected sample of stars using XMM-Newtons imagingdetectors for a total of 135 ksec. Our sample includes stars with extremelyclose-in Extrasolar Giant Planets (EGPs), with orbital radii less than 0.15 AU,as well as a control group of stars with EGPs at relatively farther distances(orbital radii greater than 2 AU). With these observations, we will be able tocharacterize and quantify the effect of close-in EGPs on stellar coronae.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-04-13T12:29:45Z/2006-06-11T03:27:26Z
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 2008-08-29T00:00:00Z
Last Update 2025-01-27
Keywords "", "stellar magnetic activity", "xmm newton", "variable governing", "extrasolar giant planets", "viz .", "sample includes stars", "XMM-Newton", "imaging detectors", "orbital radii", "XMM", "stellar coronae", "magnetic activity", "giant planets"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Vinay Kashyap, 2008, 'Extrasolar Giant Planets and Stellar Magnetic Activity', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-p9t6qup