A dataset provided by the European Space Agency

Name: The terminal braking of a relativistic jet: SS433
Published: 2005-11-11T00:00:00Z

Proposal ID	007514
Title	The terminal braking of a relativistic jet: SS433
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0075140401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0075140501
DOI	https://doi.org/10.5270/esa-46pttj9
Principal Investigator, PI	Dr Wolfgang Brinkmann
Abstract	The X-ray knots in the SNR W50 are the sides of the terminalbraking of the relativistic jets of SS433 and present a uniquelaboratory to study the physical processes by which astrophysicaljets dispose their energy into the ISM.Previous X-ray missions could neither determine the naturenor did they allow a spatially resolved spectroscopy of theemission which is a direct indicator for the energy transfer mechanism.The XMM instruments ideally match the requirements for energyrange, extent, spatial resolution, and sensitivity for this object.We propose two 25 ks pointings with the PN camera as prime instrument covering most of the eastern jet. The requested observations will allow the detailed spatially resolved spectral study of the jet - ISM interaction region.
Publications	XMM-Newton observations of the eastern jet of SS 433 \|Brinkmann W. Pratt G. W. et al. \| A&A \| 463-611 \| 2007 \| 2007A&A...463..611B \| http://ui.adsabs.harvard.edu/#abs/2007A&A...463..611B 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 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 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 Hot stars observed by XMM-Newton. I. The catalog and the properties of OB stars \|Naze Y. \| A&A \| 506-1055 \| 2009 \| 2009A&A...506.1055N \| http://ui.adsabs.harvard.edu/#abs/2009A&A...506.1055N 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 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-Zeldovich 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 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 Jets of SS 433 on scales of dozens of parsecs \|Panferov Alexander A. \| A&A \| 599-77 \| 2017 \| 2017A&A...599A..77P \| http://ui.adsabs.harvard.edu/#abs/2017A&A...599A..77P 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 Magnetic field analysis of the bow and terminal shock of the SS 433 jet \|Sakemi Haruka Machida Mami et al. \| PASJ \| 70-27 \| 2018 \| 2018PASJ...70...27S \| http://ui.adsabs.harvard.edu/#abs/2018PASJ...70...27S Very-high-energy particle acceleration powered by the jets of the microquasar SS 433 \|Abeysekara A. U. Albert A. et al. \| Natur \| 562-82 \| 2018 \| 2018Natur.562...82A \| http://ui.adsabs.harvard.edu/#abs/2018Natur.562...82A 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 The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters \|Pastor-Marazuela I. Webb N. A. et al. \| A&A \| 640-124 \| 2020 \| 2020A&A...640A.124P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...640A.124P 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 Hard X-Ray Emission from the Eastern Jet of SS 433 Powering the W50 Manatee Nebula: Evidence for Particle Reacceleration \|Safi-Harb Samar Mac Intyre Brydyn et al. \| ApJ \| 935-163 \| 2022 \| 2022ApJ...935..163S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...935..163S X-ray hot spots in the eastern ear of the supernova remnant W 50 and the microquasar SS 433 system \|Hayakawa Ryota Yamada Shinya et al. \| PASJ \| 74-510 \| 2022 \| 2022PASJ...74..510H \| http://ui.adsabs.harvard.edu/#abs/2022PASJ...74..510H X-Ray Polarization of the Eastern Lobe of SS 433 \|Kaaret Philip Ferrazzoli Riccardo et al. \| ApJ \| 961-L12 \| 2024 \| 2024ApJ...961L..12K \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961L..12K The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433 \|H. E. S. S. Collaboration Olivera-Nieto Laura et al. \| Sci \| 383-402 \| 2024 \| 2024Sci...383..402H \| http://ui.adsabs.harvard.edu/#abs/2024Sci...383..402H 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	2004-09-30T01:14:51Z/2004-10-04T09:40:44Z
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	2005-11-11T00:00:00Z
Last Update	2025-01-27
Keywords	"terminal braking", "supernova remnant w50", "energy range", "resolved spectroscopy", "xray missions", "relativistic jets", "energy transfer mechanism", "prime instrument", "xmm instruments", "pn camera", "relativistic jet", "resolved spectral", "XMM", "xray knots", "physical processes", "astrophysical jets dispose", "spatial resolution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Wolfgang Brinkmann, 2005, 'The terminal braking of a relativistic jet: SS433', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-46pttj9