A dataset provided by the European Space Agency

Name: Spectro-imagery of the supernova remnant SN1006 SSC_48
Published: 2002-09-11T00:00:00Z

Proposal ID	011109
Title	Spectro-imagery of the supernova remnant SN1006 SSC_48
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111090101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111090301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111090401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111090501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111090601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111090701
DOI	https://doi.org/10.5270/esa-x9yyevv
Principal Investigator, PI	Dr Michael Watson
Abstract	GT_SN 1006 was shown by ASCA/SIS to be of a composite nature, with non-thermal emission coming from the bright limbs and fainter thermal emission coming from the center and the other sides. This is the best example of shock acceleration of cosmic-rays (supernova remnants are thought to be the main sites of cosmic-ray acceleration). XMM has about 10 times better spatial resolution than ASCA, and will provide much crisper images. We propose to map SN 1006 in four pointings (the remnantis 30. in diameter). With 5 ks pointings we expect about 500 EPIC cts/arcmin2 in the faintest areas (10 times that in the bright limbs).
Publications	Geometry of the non-thermal emission in SN 1006. Azimuthal variations of cosmic-ray acceleration \|Rothenflug, R., Ballet, J., et al. \| A&A \| 425-121 \| 2004 \| 2004A&A...425..121R \| http://ui.adsabs.harvard.edu/#abs/2004A&A...425..121R The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The gas density around SN 1006 \|Acero, F., Ballet, J., \| A&A \| 475-883 \| 2007 \| 2007A&A...475..883A \| http://ui.adsabs.harvard.edu/#abs/2007A&A...475..883A 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 Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006 \|Miceli, M., Bocchino, F., et al. \| A&A \| 501-239 \| 2009 \| 2009A&A...501..239M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...501..239M The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/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 \| 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 The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P Shock-Cloud Interaction and Particle Acceleration in the Southwestern Limb of SN 1006 \|Miceli, M., Acero, F., et al. \| ApJ \| 782-33 \| 2014 \| 2014ApJ...782L..33M \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...782L..33M 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 Predicted gamma-ray image of SN 1006 due to inverse Compton emission \|Petruk, O., Bocchino, F., et al. \| MNRAS \| 399-157 \| 2009 \| 2009MNRAS.399..157P \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.399..157P Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X 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 Shocks and particle acceleration in supernova remnants: observational features \|Vink, Jacco, \| AdSpR \| 33-356 \| 2004 \| 2004AdSpR..33..356V \| http://ui.adsabs.harvard.edu/#abs/2004AdSpR..33..356V 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 First detection of VHE gamma-rays from SN 1006 by HESS \|Acero, F., Aharonian, F., et al. \| A&A \| 516-62 \| 2010 \| 2010A&A...516A..62A \| http://ui.adsabs.harvard.edu/#abs/2010A&A...516A..62A Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V 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 Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T 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 Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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 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 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	2000-08-17T10:35:19Z/2001-08-08T08:44:10Z
Version	PPS_NOT_AVAILABLE
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	2002-09-11T00:00:00Z
Keywords	"fainter thermal emission", "main sites", "XMM", "epic cts", "bright limbs", "shock acceleration", "nonthermal emission", "crisper images", "spectro imagery", "EPIC", "spatial resolution", "cosmic ray acceleration"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Michael Watson, 2002, 'Spectro-imagery of the supernova remnant SN1006 SSC_48', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-x9yyevv