A dataset provided by the European Space Agency

Name 011288
Title X-ray spectra and metal abundances of stars across the H-R diagram
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112880101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112880201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112880301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112880401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112880501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112880601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112880701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112880801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112880901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112881001

DOI https://doi.org/10.5270/esa-l7if11z
Author Dr Bernd Aschenbach
Description GT- We want to use the XMM EPIC camera to observe a carefully selected sample of cool stars located on key positions in the H-R diagram, MS and pre-MS stars. The goal of our observations is to obtain good S-N spectra and metal abundances of one example of each of the different classes of stars. Our observations on Algol and YY Gem are time-critical for simultaneous observations with Chandra. On Algol and CF Tuc, we request continuous observations centered on a primary eclipse. On YY Gem, our observation should be continuous, too, to cover the full orbit. HR 1084 is a calibration target for "stray light monitoring with the transparent filter", but we need to do our GT observation with the thin filter.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-07-09T11:30:43Z/2003-01-19T15:28:02Z
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 2004-02-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-02-20T00:00:00Z, 011288, 17.56_20190403_1200. https://doi.org/10.5270/esa-l7if11z