A dataset provided by the European Space Agency

Name: COMPLETING OUR UNDERSTANDING OF RCW 86
Published: 2005-04-16T00:00:00Z

Proposal ID	020800
Title	COMPLETING OUR UNDERSTANDING OF RCW 86
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0208000101
DOI	https://doi.org/10.5270/esa-9n9oet6
Principal Investigator, PI	Dr JACCO VINK
Abstract	(see original Chandra form for details)We propose to complete the mapping of the SNR RCW 86 with two observations ofthenorthern shell with both Chandra and XMM-Newton.
Publications	The X-Ray Synchrotron Emission of RCW 86 and the Implications for Its Age \|Vink, Jacco, Bleeker, Johan, et al. \| ApJ \| 648-33 \| 2006 \| 2006ApJ...648L..33V \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...648L..33V 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 A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations \|Muno, M. P., Gaensler, B. M., et al. \| ApJ \| 680-639 \| 2008 \| 2008ApJ...680..639M \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...680..639M 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 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 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 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 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 H.E.S.S. observations of the supernovae remnant RCW 86 \|Hoppe, S., Lemoine-Goumard, M., \| ICRC \| 2-585 \| 2008 \| 2008ICRC....2..585H \| http://ui.adsabs.harvard.edu/#abs/2008ICRC....2..585H 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 Teraelectronvolt Astronomy \|Hinton, J. A., Hofmann, W., \| ARA&A \| 47-523 \| 2009 \| 2009ARA&A..47..523H \| http://ui.adsabs.harvard.edu/#abs/2009ARA&A..47..523H 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 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 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	2004-01-26T22:30:59Z/2004-01-27T15:12:51Z
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	2005-04-16T00:00:00Z
Keywords	"rcw 86", "XMM", "original chandra form", "XMM-Newton", "northern shell", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr JACCO VINK, 2005, 'COMPLETING OUR UNDERSTANDING OF RCW 86', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9n9oet6