A dataset provided by the European Space Agency

Name: High Resolution X-ray Spectroscopy of the Remnant of SN 185
Published: 2008-10-01T00:00:00Z

Proposal ID	050481
Title	High Resolution X-ray Spectroscopy of the Remnant of SN 185
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504810101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504810201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504810301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504810401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504810501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504810601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0504810701
DOI	https://doi.org/10.5270/esa-vb3vyfx
Principal Investigator, PI	Dr Jacco Vink
Abstract	RCW 86/SN185 is one of the few shell-type remnants with X-ray synchrotronradiation. The remnant has a strong contrast in densities and probably also inshock velocities. In order to characterize both the thermal and non-thermalemission, we propose a large program with several deep pointings, chosen suchthat high resolution spectroscopy with the RGS is possible. This waytemperatures can be measured using single ion spectroscopy, therebycircumventing the confusion caused by the simultenuous presence of thermal andnon-thermal continuum. XMM-Newton.s RGS instrument is unique in its capabilityto obtain the high resolution spectra necessary for our goals, even for sourceextents of a few arcmin.
Publications	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 Discovery of Gamma-Ray Emission From the Shell-Type Supernova Remnant RCW 86 With Hess \|Aharonian, F., Akhperjanian, A. G., et al. \| ApJ \| 692-1500 \| 2009 \| 2009ApJ...692.1500A \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...692.1500A 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 Temperature Equilibration Behind the Shock Front: An Optical and X-Ray Study Of RCW 86 \|Helder, E. A., Vink, J., \| ApJ \| 737-85 \| 2011 \| 2011ApJ...737...85H \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...737...85H 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 Constraints on cosmic-ray efficiency in the supernova remnant RCW 86 using multi-wavelength observations \|Lemoine-Goumard, M., Renaud, M., et al. \| A&A \| 545-28 \| 2012 \| 2012A&A...545A..28L \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..28L 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 Statistical Properties of Galactic delta Scuti Stars: Revisited \|Chang, S.-W., Protopapas, P., et al. \| AJ \| 145-132 \| 2013 \| 2013AJ....145..132C \| http://ui.adsabs.harvard.edu/#abs/2013AJ....145..132C The many sides of RCW 86: a Type Ia supernova remnant evolving in its progenitor.s wind bubble \|Broersen, Sjors, Chiotellis, Alexandros, et al. \| MNRAS \| 441-3040 \| 2014 \| 2014MNRAS.441.3040B \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.441.3040B 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 Optical and X-ray observations of candidate isolated neutron stars in the G315.4-2.3 supernova remnant \|Mignani, R. P., Tiengo, A., \| MNRAS \| 425-2309 \| 2012 \| 2012MNRAS.425.2309M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.425.2309M 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 Deep Morphological and Spectral Study of the SNR RCW 86 with Fermi-LAT \|Ajello, M., Baldini, L., et al. \| ApJ \| 819-98 \| 2016 \| 2016ApJ...819...98A \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819...98A Infrared Supernova Remnants and their Infrared-to-X-ray Flux Ratios \|Koo, Bon-Chul, Lee, Jae-Joon, et al. \| ApJ \| 821-20 \| 2016 \| 2016ApJ...821...20K \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...821...20K 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 RCW 86: A Type Ia Supernova in a Wind-blown Bubble \|Williams, Brian J., Blair, William P., et al. \| ApJ \| 741-96 \| 2011 \| 2011ApJ...741...96W \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...741...96W Interstellar gas and X-rays toward the Young supernova remnant RCW 86; pursuit of the origin of the thermal and non-thermal X-ray \|Sano, H., Reynoso, E. M., et al. \| JHEAp \| 15-1 \| 2017 \| 2017JHEAp..15....1S \| http://ui.adsabs.harvard.edu/#abs/2017JHEAp..15....1S 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 Detailed spectral and morphological analysis of the shell type supernova remnant RCW 86 \|H.E.S.S. Collaboration, Abramowski, A., et al. \| A&A \| 612-4 \| 2018 \| 2018A&A...612A...4H \| http://ui.adsabs.harvard.edu/#abs/2018A&A...612A...4H 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 Possible Evidence for Cosmic-Ray Acceleration in the Type Ia SNR RCW 86: Spatial Correlation between TeV Gamma-Rays and Interstellar Atomic Protons \|Sano, H., Rowell, G., et al. \| ApJ \| 876-37 \| 2019 \| 2019ApJ...876...37S \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...876...37S 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 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 Surviving companions of Type Ia supernovae: theory and observations \|Ruiz-Lapuente, Pilar, \| NewAR \| 85-101523 \| 2019 \| 2019NewAR..8501523R \| http://ui.adsabs.harvard.edu/#abs/2019NewAR..8501523R 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 Evolutionary Models for 43 Galactic Supernova Remnants with Distances and X-Ray Spectra \|Leahy, D. A., Ranasinghe, S., \| ApJS \| 248-16 \| 2020 \| 2020ApJS..248...16L \| http://ui.adsabs.harvard.edu/#abs/2020ApJS..248...16L 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 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	2007-07-28T07:45:25Z/2007-08-25T23:34:05Z
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	2008-10-01T00:00:00Z
Keywords	"resolution spectroscopy", "shock velocities", "rgs instrument", "deep pointings", "XMM-Newton", "shell type remnant", "xmm newton", "rcw 86", "xray synchrotron radiation", "resolution xray spectroscopy", "single ion spectroscopy", "nonthermal continuum", "nonthermal emission", "source extents", "XMM", "simultenuous presence", "remnant ofsupernova185", "thereby circumventing", "resolution spectra"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jacco Vink, 2008, 'High Resolution X-ray Spectroscopy of the Remnant of SN 185', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vb3vyfx