A dataset provided by the European Space Agency

Name: Energy partition in SN 1006: thermal gas comma relativistic particles comma magnetic field
Published: 2010-04-01T00:00:00Z

Proposal ID	055563
Title	Energy partition in SN 1006: thermal gas, relativistic particles, magnetic field
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555630101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555630201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555630301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555630401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555630501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555630601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555631001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555631101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0555631201
DOI	https://doi.org/10.5270/esa-xewpkga
Principal Investigator, PI	Dr Anne Decourchelle
Abstract	We propose to carry out a deep 1 Ms XMM-Newton observation of the entire SN 1006supernova remnant (SNR) for a major breakthrough in answering key questions onthe physics of SNRs, related to particle acceleration at their shock, magneticfield amplification, heating of the electrons and ions at the shock, abundancesand distribution of the chemical elements in the ejecta. This historical type IaSNR exhibits a dual nature in X-rays with a bipolar non-thermal morphology likein radio, superposed on a fainter extended thermal emission. It is one of thebest examples of shock acceleration of cosmic-ray electrons to energiesapproaching the knee.. of the cosmic-ray spectrum and gathers the mostimportant issues concerning SNR physics.
Publications	An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L XMM-Newton evidence of shocked ISM in SN 1006: indications of hadronic acceleration \|Miceli, M., Bocchino, F., et al. \| A&A \| 546-66 \| 2012 \| 2012A&A...546A..66M \| http://ui.adsabs.harvard.edu/#abs/2012A&A...546A..66M The northwestern ejecta knot in SN 1006 \|Broersen, S., Vink, J., et al. \| A&A \| 552-9 \| 2013 \| 2013A&A...552A...9B \| http://ui.adsabs.harvard.edu/#abs/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 al. \| A&A \| 556-80 \| 2013 \| 2013A&A...556A..80M \| http://ui.adsabs.harvard.edu/#abs/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 al. \| AN \| 335-252 \| 2014 \| 2014AN....335..252M \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..252M The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/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 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y XMM-Newton large program on SN1006 - I. Methods and initial results of spatially resolved spectroscopy \|Li, Jiang-Tao, Decourchelle, Anne, et al. \| MNRAS \| 453-3953 \| 2015 \| 2015MNRAS.453.3953L \| http://ui.adsabs.harvard.edu/#abs/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 al. \| A&A \| 593-26 \| 2016 \| 2016A&A...593A..26M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..26M XMM-Newtonlarge programme on SN1006 - II. Thermal emission \|Li, Jiang-Tao, Decourchelle, Anne, et al. \| MNRAS \| 462-158 \| 2016 \| 2016MNRAS.462..158L \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.462..158L The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Detection of Two TeV Shell-type Remnants at GeV Energies with FERMI LAT: HESS J1731-347 and SN 1006 \|Condon, B., Lemoine-Goumard, M., et al. \| ApJ \| 851-100 \| 2017 \| 2017ApJ...851..100C \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...851..100C Spatially Resolved Broadband Synchrotron Emission from the Nonthermal Limbs of SN1006 \|Li, Jiang-Tao, Ballet, Jean, et al. \| ApJ \| 864-85 \| 2018 \| 2018ApJ...864...85L \| http://ui.adsabs.harvard.edu/#abs/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 al. \| ApJ \| 879-64 \| 2019 \| 2019ApJ...879...64S \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...879...64S Fermi LAT detection of the supernova remnant SN 1006 revisited: The southwest limb \|Xing, Yi, Wang, Zhongxiang, et al. \| PASJ \| 71-77 \| 2019 \| 2019PASJ...71...77X \| http://ui.adsabs.harvard.edu/#abs/2019PASJ...71...77X Erratum: .XMM-newton large program on SN1006 - II: Thermal emission. (2016, MNRAS, 462, 158) \|Li, Jiang-Tao, Decourchelle, Anne, et al. \| MNRAS \| 499-862 \| 2020 \| 2020MNRAS.499..862L \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 499-5679 \| 2020 \| 2020MNRAS.499.5679L \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.499.5679L Modeling particle acceleration and non-thermal emission in supernova remnants \|Orlando, S., Miceli, M., et al. \| NewA \| 86-101566 \| 2021 \| 2021NewA...8601566O \| http://ui.adsabs.harvard.edu/#abs/2021NewA...8601566O Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca, A., Salvaterra, R., et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D The supernova remnant SN 1006 as a Galactic particle accelerator \|Giuffrida, Roberta, Miceli, Marco, et al. \| NatCo \| 13-5098 \| 2022 \| 2022NatCo..13.5098G \| http://ui.adsabs.harvard.edu/#abs/2022NatCo..13.5098G Magnetic Structures and Turbulence in SN 1006 Revealed with Imaging X-Ray Polarimetry \|Zhou, Ping, Prokhorov, Dmitry, et al. \| ApJ \| 957-55 \| 2023 \| 2023ApJ...957...55Z \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...957...55Z From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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 Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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
Keywords	"magnetic field", "thermal gas", "supernova remnant", "cosmic ray electrons", "supernova remnant physics", "XMM-Newton", "chemical elements", "particle acceleration", "thermal emission", "bipolar nonthermal morphology", "answering key", "energy partition insupernova1006", "XMM", "magnetic field amplification", "energies approaching", "cosmic ray spectrum", "ms xmm newton", "relativistic particles", "major breakthrough", "knee ''", "shock acceleration"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Anne Decourchelle, 2010, 'Energy partition in SN 1006: thermal gas comma relativistic particles comma magnetic field', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xewpkga