A dataset provided by the European Space Agency

Name: THE EVOLUTION OF CTB109
Published: 2003-08-09T00:00:00Z

Proposal ID	005754
Title	THE EVOLUTION OF CTB109
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057540101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057540201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057540301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057540401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0057540601
DOI	https://doi.org/10.5270/esa-h126gcz
Principal Investigator, PI	Dr Paul Plucinsky
Abstract	The supernova remnant (SNR) CTB109 presents a unique laboratory for studying theinteraction of SNRs with interstellar clouds: one half of the remnant has expanded unimpeded into a low-density medium and the other half has expanded directly into a dense molecular cloud. The nearly ideal viewing geometry allowsthe two halves to be cleanly separated. The spectrum of the outer shell, the bright interior emission, and the shock/cloud interface will be well characterized by the three proposed 15 ks pointings. We will determine the ionization structure as a function of position behind the shock, as well asmeasuring the temperature and abundances. Despite being observed by every majorX-ray observatory, there still exists much uncertainty in the physical ..
Publications	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 Long-term Radiative Evolution of Anomalous X-Ray Pulsar 1E 2259+586 After its 2002 Outburst \|Zhu, Weiwei, Kaspi, Victoria M., et al. \| ApJ \| 686-520 \| 2008 \| 2008ApJ...686..520Z \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...686..520Z XMM-Newton Observations of the Galactic Supernova Remnant CTB 109 (G109.1-1.0) \|Sasaki, Manami, Plucinsky, Paul P., et al. \| ApJ \| 617-322 \| 2004 \| 2004ApJ...617..322S \| http://ui.adsabs.harvard.edu/#abs/2004ApJ...617..322S 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 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 Fermi-LAT Observations and a Broadband Study of Supernova Remnant CTB 109 \|Castro, Daniel, Slane, Patrick, et al. \| ApJ \| 756-88 \| 2012 \| 2012ApJ...756...88C \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...88C 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 Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey \|Pineau, F.-X., Motch, C., et al. \| A&A \| 527-126 \| 2011 \| 2011A&A...527A.126P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.126P Exploring X-ray and radio emission of type 1 AGN up to z virgul 2.3 \|Ballo, L., Heras, F. J. H., et al. \| A&A \| 545-66 \| 2012 \| 2012A&A...545A..66B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca, A., Molendi, S., \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L 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 Comparing supernova remnants around strongly magnetized and canonical pulsars \|Martin, J., Rea, N., et al. \| MNRAS \| 444-2910 \| 2014 \| 2014MNRAS.444.2910M \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444.2910M X-Ray Perspective of the Twisted Magnetospheres of Magnetars \|Weng, Shan-Shan, Gogus, Ersin, et al. \| ApJ \| 805-81 \| 2015 \| 2015ApJ...805...81W \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...805...81W 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 Changes in the X-Ray Emission from the Magnetar Candidate 1E 2259+586 during Its 2002 Outburst \|Woods, P. M., Kaspi, V. M., et al. \| ApJ \| 605-378 \| 2004 \| 2004ApJ...605..378W \| http://ui.adsabs.harvard.edu/#abs/2004ApJ...605..378W 3D hydrodynamic simulations of the Galactic supernova remnant CTB 109 \|Bolte, J., Sasaki, M., \| A&A \| 582-47 \| 2015 \| 2015A&A...582A..47B \| http://ui.adsabs.harvard.edu/#abs/2015A&A...582A..47B 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 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 The Spectrum of the Universe \|Hill, Ryley, Masui, Kiyoshi W., \| ApSpe \| 72-663 \| 2018 \| 2018ApSpe..72..663H \| http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H 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 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 A Spectroscopic Study of Supernova Remnants with the Infrared Space Observatory \|Millard, Matthew J., Ravi, Aravind P., et al. \| ApJS \| 257-36 \| 2021 \| 2021ApJS..257...36M \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..257...36M Correlation Study of Temporal and Emission Properties of Quiescent Magnetars \|Seo, Jiwoo, Lee, Jaewon, \| JKAS \| 56-41 \| 2023 \| 2023JKAS...56...41S \| http://ui.adsabs.harvard.edu/#abs/2023JKAS...56...41S 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	2002-01-22T15:51:17Z/2002-07-09T18:28:59Z
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	2003-08-09T00:00:00Z
Keywords	"physical ...", "major xray observatory", "supernova remnant", "dense molecular cloud", "outer shell", "cleanly separated", "nearly ideal", "bright interior emission", "low density medium", "geometry allows", "expanded unimpeded", "ionization structure", "interstellar clouds", "cloud interface"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Paul Plucinsky, 2003, 'THE EVOLUTION OF CTB109', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-h126gcz