A dataset provided by the European Space Agency

Name 040200
Title Candidates for low-luminosity supersoft sources in the Magellanic Clouds
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402000101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402000201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402000501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402000601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402000701

DOI https://doi.org/10.5270/esa-ntwflnt
Author European Space Agency
Description We propose XMM-Newton observations of new candidate supersoft X-ray sources,
SSSs, in the Magellanic Clouds, MCs, in order to confirm and study their nature.
The 20 ks exposures will allow to determine a precise position, spectral and
temporal investigations. Finding new SSS in the MCs is crucial for X-ray source
population studies and will provide new information on the physics of individual
objects and on the class of SSSs as such. In particular we will address the
question if persistent low-luminosity SSSs exist, which is not easily to
understand in the framework of stable burning at high accretion rates, or if
they are highly variable.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-08-29T10:28:40Z/2007-01-29T00:00:11Z
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 2008-03-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008, Candidates For Low-Luminosity Supersoft Sources In The Magellanic Clouds, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ntwflnt