A dataset provided by the European Space Agency

Name 055563
Title Energy partition in SN 1006: thermal gas, relativistic particles, magnetic field
URL

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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555630201
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http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555630401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555630501
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DOI 10.5270/esa-xewpkga
Author Dr Anne Decourchelle
Description We propose to carry out a deep 1 Ms XMM-Newton observation of the entire SN 1006 supernova remnant (SNR) for a major breakthrough in answering key questions on the physics of SNRs, related to particle acceleration at their shock, magnetic field amplification, heating of the electrons and ions at the shock, abundances and distribution of the chemical elements in the ejecta. This historical type Ia SNR exhibits a dual nature in X-rays with a bipolar non-thermal morphology like in radio, superposed on a fainter extended thermal emission. It is one of the best examples of shock acceleration of cosmic-ray electrons to energies approaching the "knee.. of the cosmic-ray spectrum and gathers the most important issues concerning SNR physics.
Publication An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
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 . 2012 . 2012ApJ...756...27L ,
XMM-Newton evidence of shocked ISM in SN 1006: indications of hadronic acceleration . Miceli, M., Bocchino, F., et all. . A&A . 546-66 . 2012 . 2012A&A...546A..66M ,
The northwestern ejecta knot in SN 1006 . Broersen, S., Vink, J., et all. . A&A . 552-9 . 2013 . 2013A&A...552A...9B ,
The shape of the cutoff in the synchrotron emission of SN 1006 observed with XMM-Newton . Miceli, M., Bocchino, F., et all. . A&A . 556-80 . 2013 . 2013A&A...556A..80M ,
The loss-limited electron energy in SN 1006: Effects of the shock velocity and of the diffusion process . Miceli, M., Bocchino, F., et all. . AN . 335-252 . 2014 . 2014AN....335..252M ,
The diversity of quasars unified by accretion and orientation . Shen, Yue, Ho, Luis C., . Natur . 513-210 . 2014 . 2014Natur.513..210S ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . ...,
XMM-Newton large program on SN1006 - I. Methods and initial results of spatially resolved spectroscopy . Li, Jiang-Tao, Decourchelle, Anne, et all. . MNRAS . 453-3953 . 2015 . 2015MNRAS.453.3953L ,
Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and gamma-ray emission . Miceli, M., Orlando, S., et all. . A&A . 593-26 . 2016 . 2016A&A...593A..26M ,
XMM-Newtonlarge programme on SN1006 - II. Thermal emission . Li, Jiang-Tao, Decourchelle, Anne, et all. . MNRAS . 462-158 . 2016 . 2016MNRAS.462..158L ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Detection of Two TeV Shell-type Remnants at GeV Energies with FERMIÂxa0LAT: HESS J1731-347 and SN 1006 . Condon, B., Lemoine-Goumard, M., et all. . ApJ . 851-100 . 2017 . 2017ApJ...851..100C ,
Spatially Resolved Broadband Synchrotron Emission from the Nonthermal Limbs of SN1006 . Li, Jiang-Tao, Ballet, Jean, et all. . ApJ . 864-85 . 2018 . 2018ApJ...864...85L ,
Genus Statistic Applied to the X-Ray Remnant of SN 1572: Clues to the Clumpy Ejecta Structure of Type Ia Supernovae . Sato, Toshiki, Hughes, John P., et all. . ApJ . 879-64 . 2019 . 2019ApJ...879...64S ,
Fermi LAT detection of the supernova remnant SN 1006 revisited: The southwest limb . Xing, Yi, Wang, Zhongxiang, et all. . PASJ . 71-77 . 2019 . 2019PASJ...71...77X ,
Erratum: .XMM-newton large program on SN1006 - II: Thermal emission. (2016, MNRAS, 462, 158) . Li, Jiang-Tao, Decourchelle, Anne, et all. . MNRAS . 499-862 . 2020 . 2020MNRAS.499..862L ,
Erratum: XMM-Newton large program on SN1006 - I. Methods and initial results of spatially resolved spectroscopy . Li, Jiang-Tao, Decourchelle, Anne, et all. . MNRAS . 499-5679 . 2020 . 2020MNRAS.499.5679L ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2008-07-31T03:42:44Z/2009-02-21T03:45:38Z
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 2010-04-01T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-04-01T00:00:00Z, 055563, 17.56_20190403_1200. https://doi.org/10.5270/esa-xewpkga