A dataset provided by the European Space Agency

Name 060082
Title Coronal activity cycles in solar analog stars
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600820401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600820501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600820601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600820701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600820801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600820901

DOI https://doi.org/10.5270/esa-xum1bx0
Author Dr Fabio Favata
Description The present program to detect and 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 from 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. The present proposal requests continuation of the ongoing monitoring program into XMM AO-8, needed to progress toward full characterization of the coronal cycle for our targets. The most observed of our targets (HD 81809) will enter its cycle maximum during the XMM AO-8 period, and given the higher variability expected at maximum, we request a more frequent sampling for this target.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-05-24T23:00:31Z/2010-05-01T03:03:47Z
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 2011-05-21T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011, 060082, 17.56_20190403_1200. https://doi.org/10.5270/esa-xum1bx0