A dataset provided by the European Space Agency

Name 067032
Title Coronal activity cycles in solar analog stars
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670320101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670320201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670320301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670320601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0670320701

DOI https://doi.org/10.5270/esa-v84qo2x
Author European Space Agency
Description The present program to study for the first time solar-like cycles in the X-ray
emission of stars similar to our Sun has been ongoing since XMM s AO-1. Five
targets in three stellar systems have been monitored since 2001, providing for
the first time clear evidence of long-term cycles in the X-ray luminosity of
normal stars, with variations in X-ray luminosity of up to an order of
magnitude. We request continuation of the ongoing monitoring program into XMM
AO-10, needed to progress toward full characterization of the coronal cycle for
our targets.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-11-02T00:53:03Z/2012-05-07T15:56:21Z
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 2013-05-18T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, Coronal Activity Cycles In Solar Analog Stars, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-v84qo2x