A dataset provided by the European Space Agency

Name 050147
Title Candidates for low-luminosity supersoft sources in the Magellanic Clouds
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0501470101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0501470201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0501470501

DOI 10.5270/esa-iqjwg8e
Author Dr Frank Haberl
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 and 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 XMM-Newton observations of the Small Magellanic Cloud: Be-X-ray binary pulsars active between October 2006 and June 2007 . Haberl, F., Eger, P., . A&A . 489-327 . 2008 . 2008A&A...489..327H ,
Quasi-stellar Object Selection Algorithm Using Time Variability and Machine Learning: Selection of 1620 Quasi-stellar Object Candidates from MACHO Large Magellanic Cloud Database . Kim, Dae-Won, Protopapas, Pavlos, et all. . ApJ . 735-68 . 2011 . 2011ApJ...735...68K ,
A Refined QSO Selection Method Using Diagnostics Tests: 663 QSO Candidates in the Large Magellanic Cloud . Kim, Dae-Won, Protopapas, Pavlos, et all. . ApJ . 747-107 . 2012 . 2012ApJ...747..107K ,
An XMM-Newton view of planetary nebulae in the Small Magellanic Cloud. The X-ray luminous central star of SMP SMC 22 . Mereghetti, S., Krachmalnicoff, N., et all. . A&A . 519-42 . 2010 . 2010A&A...519A..42M ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Highly absorbed X-ray binaries in the Small Magellanic Cloud . Novara, G., La Palombara, N., et all. . A&A . 532-153 . 2011 . 2011A&A...532A.153N ,
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 Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 ....
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-05-14T14:41:28Z/2007-06-04T18:20:49Z
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 2008-06-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-06-23T00:00:00Z, 050147, 17.56_20190403_1200. https://doi.org/10.5270/esa-iqjwg8e