A dataset provided by the European Space Agency

Name: Study of the X-ray baffle leak using an extended source - 1
Published: 2001-12-27T00:00:00Z

Proposal ID	009621
Title	Study of the X-ray baffle leak using an extended source - 1
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0096210101
DOI	https://doi.org/10.5270/esa-9bydm80
Principal Investigator, PI	Dr Bernd Aschenbach
Abstract	PV- X-rays from sources outside the field of view can enter the EPIC field of view. The X-ray baffles in front still leak at some level out to off-axis anglesof about 1.5 degrees. The angular dependence and the level have been measured onground but need to be verified in orbit by one pointing with the source on-axisand four additional pointings with the source offset by 70 arcmin at fourdifferent azimuth angles. The source should be sufficiently bright, stable intime and should show emission lines to ease the analysis of the spectraldependence. A moderate spatial extent but less than the EPIC field of view isadvantageous. Such a source is the Tycho SNR. This proposal is for the on-axisposition of the programme.
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 Inner-shell ionization radiative losses and thermal conductivity in young SNRs \|Kosenko D. I. \| MNRAS \| 369-1407 \| 2006 \| 2006MNRAS.369.1407K \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.369.1407K XMM-Newton observation of the Tycho supernova remnant \|Decourchelle A. Sauvageot J. L. et al. \| A&A \| 365-218 \| 2001 \| 2001A&A...365L.218D \| http://ui.adsabs.harvard.edu/#abs/2001A&A...365L.218D Constraints on the Physics of Type Ia Supernovae from the X-Ray Spectrum of the Tycho Supernova Remnant \|Badenes Carles Borkowski Kazimierz J. et al. \| ApJ \| 645-1373 \| 2006 \| 2006ApJ...645.1373B \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...645.1373B 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 X-ray spectroscopy of supernova remnants \|Ballet Jean Decourchelle Anne \| NewAR \| 46-507 \| 2002 \| 2002NewAR..46..507B \| http://ui.adsabs.harvard.edu/#abs/2002NewAR..46..507B 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 Modelling the interaction of thermonuclear supernova remnants with circumstellar structures: the case of Tychos supernova remnant \|Chiotellis A. Kosenko D. et al. \| MNRAS \| 435-1659 \| 2013 \| 2013MNRAS.435.1659C \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.435.1659C 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 Discovery of a 3.5 keV line in the Galactic Centre and a critical look at the origin of the line across astronomical targets \|Jeltema Tesla Profumo Stefano \| MNRAS \| 450-2143 \| 2015 \| 2015MNRAS.450.2143J \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.450.2143J Spatial Distribution of X-Ray Emitting Ejecta in Tychos SNR: Indications of Shocked Titanium \|Miceli M. Sciortino S. et al. \| ApJ \| 805-120 \| 2015 \| 2015ApJ...805..120M \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...805..120M 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 Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus \|Carlson Eric Jeltema Tesla \| JCAP \| 2-9 \| 2015 \| 2015JCAP...02..009C \| http://ui.adsabs.harvard.edu/#abs/2015JCAP...02..009C 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 A study of Tychos SNR at TeV energies with the HEGRA CT-System \|Aharonian F. A. Akhperjanian A. G. et al. \| A&A \| 373-292 \| 2001 \| 2001A&A...373..292A \| http://ui.adsabs.harvard.edu/#abs/2001A&A...373..292A 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 Thermal X-Ray Emission From Young Type Ia Supernova Remnants \|Badenes Carles \| PhDT \| 0-27 \| 2004 \| 2004PhDT........27B \| http://ui.adsabs.harvard.edu/#abs/2004PhDT........27B High Resolution X-ray Observations of Supernova Remnants \|Bocchino F. \| ChJAS \| 3-329 \| 2003 \| 2003ChJAS...3..329B \| http://ui.adsabs.harvard.edu/#abs/2003ChJAS...3..329B 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 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
Instrument	EMOS1, EMOS2, EPN, RGS1, RGS2
Temporal Coverage	2000-06-29T02:50:21Z/2000-06-29T17:35:10Z
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	2001-12-27T00:00:00Z
Last Update	2025-01-27
Keywords	"emission lines", "tycho supernova remnant", "axis angles", "EPIC", "axis position", "azimuth angles", "source offset", "epic field", "additional pointings", "moderate spatial extent", "xray baffles", "xray baffle leak"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Bernd Aschenbach, 2001, 'Study of the X-ray baffle leak using an extended source - 1', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-9bydm80