A dataset provided by the European Space Agency

Name: Snap-Shot Survey of Supernova Remnants with Plerionic Components
Published: 2007-05-31T00:00:00Z

Proposal ID	030188
Title	Snap-Shot Survey of Supernova Remnants with Plerionic Components
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301880101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301880201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301880301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301880401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301880501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301880601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301880901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301881001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301881101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301881201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0301881301 ...
DOI	https://doi.org/10.5270/esa-1mwvu7h
Principal Investigator, PI	Dr Oleg Kargaltsev
Abstract	Supernova Remnants of center-filled and composite types often host young,energetic pulsars emitting strong relativistic winds. XMM-Newton and Chandraobservations of such SNRs have already resulted in a number of pulsar andpulsar-wind nebula (PWN) discoveries. We propose to observe the remainingplerionic remnants located within a distance of 7 kpc. The SNRs were selectedbased on their radio morphologies and serendipitous ROSAT or ASCA data. Thissurvey will substantially expand the sample of PNWe and pulsars observed inX-rays and help to establish the properties of the overall population.
Publications	Searching for Compact Objects in SNRs G27.8+0.6 and G28.8+1.5 \|Misanovic, Zdenka, Kargaltsev, Oleg, \| ApJ \| 725-931 \| 2010 \| 2010ApJ...725..931M \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...725..931M 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 first X-ray survey of Galactic luminous blue variables \|Naze, Y., Rauw, G., \| A&A \| 538-47 \| 2012 \| 2012A&A...538A..47N \| http://ui.adsabs.harvard.edu/#abs/2012A&A...538A..47N 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 The Galactic plane at faint X-ray fluxes - I. Properties and characteristics of the X-ray source population \|Warwick, R. S., Perez-Ramirez, D., \| MNRAS \| 413-595 \| 2011 \| 2011MNRAS.413..595W \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.413..595W 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 The Galactic plane at faint X-ray fluxes - II. Stacked X-ray spectra of a sample of serendipitous XMM-Newton sources \|Warwick, R. S., Byckling, K., \| MNRAS \| 438-2967 \| 2014 \| 2014MNRAS.438.2967W \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438.2967W 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 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 The high-energy gamma-ray detection of G73.9+0.9, a supernova remnant interacting with a molecular cloud \|Zdziarski, Andrzej A., Malyshev, Denys, et al. \| MNRAS \| 455-1451 \| 2016 \| 2016MNRAS.455.1451Z \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.455.1451Z 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 Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz, Tobias, \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P 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 Discovery of TeV \\u03b3-ray emission from the neighbourhood of the supernova remnant G24.7+0.6 by MAGIC \|MAGIC Collaboration, Acciari, V. A., et al. \| MNRAS \| 483-4578 \| 2019 \| 2019MNRAS.483.4578M \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.4578M 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 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 Probing the nature of the X-ray source IGR J16327-4940 with Chandra \|Sidoli, L., Sguera, V., et al. \| MNRAS \| 526-2560 \| 2023 \| 2023MNRAS.526.2560S \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.2560S 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	2005-09-14T12:15:17Z/2006-04-19T18:15:13Z
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	2007-05-31T00:00:00Z
Keywords	"energetic pulsars emitting", "plerionic components", "supernova remnant", "XMM", "xmm newton", "snap shot survey", "overall population", "asca data", "substantially expand", "center filled", "XMM-Newton", "radio morphologies", "composite types", "ROSAT", "relativistic winds", "plerionic remnant located"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Oleg Kargaltsev, 2007, 'Snap-Shot Survey of Supernova Remnants with Plerionic Components', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-1mwvu7h