A dataset provided by the European Space Agency

Name: SN 1006: A Laboratory for Cosmic Ray Acceleration
Published: 2002-11-15T00:00:00Z

Proposal ID	007734
Title	SN 1006: A Laboratory for Cosmic Ray Acceleration
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0077340101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0077340201
DOI	https://doi.org/10.5270/esa-gkgj9v2
Principal Investigator, PI	Dr Jacco Vink
Abstract	We propose to observe SN 1006 with the RGS as prime instrument using twopointings of each 50virgulks. We will use spectroscopic diagnostics to investigatethe various shock fronts around the remnant, of which the cosmic rayacceleration region on the NE limb should be particularly interesting. Electrontemperature diagnostics in He-like systems N VI and O VII (and higher, Ne IX,Mg XI if possible) will be used to search for electrons energized at the NE limbto form the population of seed particles for cosmic ray acceleration. RGSspectra will be combined with EPIC images to account as fully as possible forthe effect of the spatial extent of the source on the spectral resolution.Additionally we will use the OM to search for synchrotron radiation in theopt/UV
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 The Slow Temperature Equilibration behind the Shock Front of SN 1006 \|Vink, Jacco, Laming, J. Martin, et al. \| ApJ \| 587-31 \| 2003 \| 2003ApJ...587L..31V \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...587L..31V 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 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 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 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S 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 High Resolution X-ray Observations of Supernova Remnants \|Bocchino, F., \| ChJAS \| 3-329 \| 2003 \| 2003ChJAS...3..329B \| http://ui.adsabs.harvard.edu/#abs/2003ChJAS...3..329B 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	2001-08-10T03:59:21Z/2001-08-11T15:29:22Z
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	2002-11-15T00:00:00Z
Keywords	"seed particles", "ne ix", "sn 1006", "electrons energized", "EPIC", "spatial extent", "spectroscopic diagnostics", "shock fronts", "epic images", "mg xi", "electron temperature diagnostics", "ne limb", "synchrotron radiation", "spectral resolution", "prime instrument", "rgs spectra", "cosmic ray acceleration"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jacco Vink, 2002, 'SN 1006: A Laboratory for Cosmic Ray Acceleration', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gkgj9v2