A dataset provided by the European Space Agency

Name 020381
Title RESTLESS DAYS OF THE INFANT SUN
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203810101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0203810201

DOI 10.5270/esa-8iisanf
Author Mrs ALESSANDRA TELLESCHI
Description The earliest stages of the Sun.s life were fundamentally important for the formation of planetary seeds, physical and chemical processes in the Solar Nebula, the dissipation of left-over molecular material, the formation, distribution, and binding of water (e.g., in Oort-cloud comets, in the giant planets, or on Earth and Mars), and the chemistry of the forming planetary atmospheres. The principal goal of the present proposal is a study of the pre-main sequence high-energy life of our Sun by investigating a sample of stars of approximately one solar mass with known ages in the nearby Chamaeleon I star formation region. The large effective area of the XMM-Newton EPIC cameras allows us to conduct a spectroscopic X-ray study of the PMS X-ray Sun in Time.
Publication On the origin of [NeII] 12.81 mum emission from pre-main sequence stars: Disks, jets, and accretion . Gudel, M., Lahuis, F., et all. . A&A . 519-113 . 2010 . 2010A&A...519A.113G ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
X-ray emission of brown dwarfs: towards constraining the dependence on age, luminosity, and temperature . Stelzer, B., Micela, G., et all. . A&A . 448-293 . 2006 . 2006A&A...448..293S ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
Classification of X-Ray Sou...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-02-27T16:25:05Z/2004-09-29T02:32:21Z
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 2005-11-06T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-11-06T00:00:00Z, 020381, 17.56_20190403_1200. https://doi.org/10.5270/esa-8iisanf