A dataset provided by the European Space Agency

Name 020184
Title SINGLE ION SPECTROSCOPY OF MAGELLANIC CLOUD SNRS
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201840101

DOI 10.5270/esa-wnnyx4y
Author Mr KURT VAN DER HEYDEN
Description We propose to observe three supernova remnants in the Magellanic clouds, i.e. DEM L 71, IKT 6 & IKT 23. The RGS spectra will allow us to study the emission lines from single ions. In particular, the He-like series of O & Ne (in the case of IKT 23) show peculiar ratios. The study of the He-like ratios will enable us to investigate largely unaccounted for phenomena, such as resonance scattering, recombination and charge transfer which affects line shapes and production.
Publication 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 ,
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 ,
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 ,
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 ,
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 ,
Faint super-soft X-ray sources in XMM-Newton Large Magellanic Cloud fields . Kahabka, P., Haberl, F., et all. . A&A . 482-237 . 2008 . 2008A&A...482..237K ,
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 . <...
Instrument EPN, RGS1, OM, RGS2, EMOS1, EMOS2
Temporal Coverage 2003-12-13T20:16:36Z/2003-12-14T13:33:29Z
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 2005-01-10T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-01-10T00:00:00Z, 020184, 17.56_20190403_1200. https://doi.org/10.5270/esa-wnnyx4y