A dataset provided by the European Space Agency

Name: Completing the X-ray census of Plerionic Supernova Remnants within 7 kpc
Published: 2007-11-22T00:00:00Z

Proposal ID	040091
Title	Completing the X-ray census of Plerionic Supernova Remnants within 7 kpc
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400910101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400910201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400910301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0400910401
DOI	https://doi.org/10.5270/esa-w20i102
Principal Investigator, PI	Dr Oleg Kargaltsev
Abstract	Supernova Remnants of center-filled and composite types often host young,energetic pulsars emitting strong relativistic winds. Chandra and XMM-Newtonobservations of such SNRs have already resulted in a number of pulsar andpulsar-wind nebula (PWN) discoveries. We propose to complete the X-ray census ofplerionic remnants within a 7 kpc distance, which we have begun in XMM-NewtonAO-4. The SNRs were selected based on their radio morphologies and archivalROSAT or ASCA data. This short survey will substantially expand the sample ofPNWe and pulsars observed in X-rays and help to establish the properties of theoverall population.
Publications	XMM-Newton Observations of Two Candidate Supernova Remnants \|Kargaltsev, O., Schmitt, B. M., et al. \| ApJ \| 745-99 \| 2012 \| 2012ApJ...745...99K \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...745...99K 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 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 Long-term spectral and timing properties of the soft gamma-ray repeater SGR 1833-0832 and detection of extended X-ray emission around the radio pulsar PSR B1830-08 \|Esposito, P., Israel, G. L., et al. \| MNRAS \| 416-205 \| 2011 \| 2011MNRAS.416..205E \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.416..205E 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 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 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 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 Suzaku observations of two diffuse hard X-ray source regions, G22.0+0.0 and G23.5+0.1 \|Yamauchi, Shigeo, Sumita, Mayu, \| PASJ \| 68-6 \| 2016 \| 2016PASJ...68S...6Y \| http://ui.adsabs.harvard.edu/#abs/2016PASJ...68S...6Y 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 Systematic study of magnetar outbursts \|Coti Zelati, Francesco, Rea, Nanda, et al. \| MNRAS \| 474-961 \| 2018 \| 2018MNRAS.474..961C \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.474..961C 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 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	2006-08-13T12:25:52Z/2006-10-18T11:13:51Z
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	2007-11-22T00:00:00Z
Keywords	"supernova remnant", "XMM-Newton", "relativistic winds", "xmm newton", "xmm newton ao", "center filled", "xray census", "composite types", "ROSAT", "overall population", "XMM", "asca data", "radio morphologies", "energetic pulsars emitting", "short survey", "archival rosat", "substantially expand", "plerionic remnant", "plerionic supernova remnant"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Oleg Kargaltsev, 2007, 'Completing the X-ray census of Plerionic Supernova Remnants within 7 kpc', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-w20i102