A dataset provided by the European Space Agency

Name 008520
Title Fe K line emission of a center-filled SNR 3C397
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0085200101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0085200301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0085200401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0085200501

DOI 10.5270/esa-vmnx3fp
Author Dr Ken.ichi Torii
Description We propose to perform a 33 ks observation of the young center-filled supernova remnant (SNR) 3C397 using XMM. Observation goals are as follows: 1. Spatial mapping of Si, S and Fe lines and reveal their stratification. 2. Determine progenitor type by measuring metal abundances. 3. Study whether the thermal emission comes from the center-filled or the shell-like structure.
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 ,
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 ,
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 ,
A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations . Muno, M. P., Gaensler, B. M., et all. . ApJ . 680-639 . 2008 . 2008ApJ...680..639M ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
Spatial distribution of metal emissions in supernova remnant 3C 397 viewed with Chandra and XMM . Jiang, Bing, Chen, Yang, . SCPMA . 53-267 . 2010 . 2010SCPMA..53S.267J ,
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 Sources in the XMM-Newton Se...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-10-15T00:19:47Z/2004-04-25T19:56:05Z
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 2005-09-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2005-09-09T00:00:00Z, 008520, 17.56_20190403_1200. https://doi.org/10.5270/esa-vmnx3fp