A dataset provided by the European Space Agency

Name: Disentangling X-ray emission processes in Vela-like pulsars
Published: 2003-09-06T00:00:00Z

Proposal ID	005454
Title	Disentangling X-ray emission processes in Vela-like pulsars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0054540101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0054540501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0054540701
DOI	https://doi.org/10.5270/esa-qv4mb33
Principal Investigator, PI	Dr Bryan Gaensler
Abstract	X-ray emission from pulsars can be used to probe both thermal processes, such asneutron star cooling and the surrounding supernova blast wave, and also the non-thermal physics of a pulsar.s magnetosphere and relativistic wind. The Vela-likepulsars (ages 10-50 kyr) represent a transition between younger and older pul-sars, and are the key to understanding the evolution of these various sources ofX-ray emission. But because in these pulsars we observe all these processes atthe same time, it can be problematic to disentangle their different contributi-ons. We here propose XMM observations of four Vela-like pulsars in order to se-parate out non-thermal and thermal contributions to their emission, and to placethese energetic sources in the context of neutron star population as a whole
Publications	Identifying XMM-Newton observations affected by solar wind charge exchange - Part II \|Carter, J. A., Sembay, S., \| A&A \| 527-115 \| 2011 \| 2011A&A...527A.115C \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.115C 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 Multiwavelength Study on the High-energy Behavior of the Fermi/LAT Pulsars \|Marelli, Martino, De Luca, Andrea, \| ApJ \| 733-82 \| 2011 \| 2011ApJ...733...82M \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...733...82M A possible association of the new VHE gamma-ray source HESS J1825-137 with the pulsar wind nebula G18.0-0.7 \|Aharonian, F. A., Akhperjanian, A. G., et al. \| A&A \| 442-25 \| 2005 \| 2005A&A...442L..25A \| http://ui.adsabs.harvard.edu/#abs/2005A&A...442L..25A XMM-Newton Observations of PSR B1823-13: An Asymmetric Synchrotron Nebula around a Vela-like Pulsar \|Gaensler, B. M., Schulz, N. S., et al. \| ApJ \| 588-441 \| 2003 \| 2003ApJ...588..441G \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...588..441G Chandra and XMM-Newton Observations of the Vela-like Pulsar B1046-58 \|Gonzalez, M. E., Kaspi, V. M., et al. \| ApJ \| 652-569 \| 2006 \| 2006ApJ...652..569G \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...652..569G Chandra Observation of PSR B1823-13 and Its Pulsar Wind Nebula \|Pavlov, G. G., Kargaltsev, O., \| ApJ \| 675-683 \| 2008 \| 2008ApJ...675..683P \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...675..683P 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 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 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 A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C 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 New VLT observations of the Fermi pulsar PSR J1048-5832 \|Razzano, M., Mignani, R. P., et al. \| MNRAS \| 428-3636 \| 2013 \| 2013MNRAS.428.3636R \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.428.3636R Deep optical imaging of the gamma-ray pulsar J1048-5832 with the VLT \|Danilenko, A., Kirichenko, A., et al. \| A&A \| 552-127 \| 2013 \| 2013A&A...552A.127D \| http://ui.adsabs.harvard.edu/#abs/2013A&A...552A.127D The Second Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars \|Abdo, A. A., Ajello, M., et al. \| ApJS \| 208-17 \| 2013 \| 2013ApJS..208...17A \| http://ui.adsabs.harvard.edu/#abs/2013ApJS..208...17A 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 Suzaku Observation of HESS J1825-137: Discovery of Largely-Extended X-Rays from PSR J1826-1334 \|Uchiyama, Hideki, Matsumoto, Hironori, et al. \| PASJ \| 61-189 \| 2009 \| 2009PASJ...61S.189U \| http://ui.adsabs.harvard.edu/#abs/2009PASJ...61S.189U 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 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 Status of identification of VHE gamma-ray sources \|Funk, Stefan, \| Ap&SS \| 309-11 \| 2007 \| 2007Ap&SS.309...11F \| http://ui.adsabs.harvard.edu/#abs/2007Ap&SS.309...11F Fermi Large Area Telescope Detection of Pulsed gamma-rays from the Vela-like Pulsars PSR J1048-5832 and PSR J2229+6114 \|Abdo, A. A., Ackermann, M., et al. \| ApJ \| 706-1331 \| 2009 \| 2009ApJ...706.1331A \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...706.1331A 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 Modeling the magnetospheric X-ray emission from solar wind charge exchange with verification from XMM-Newton observations \|Whittaker, Ian C., Sembay, Steve, et al. \| JGRA \| 121-4158 \| 2016 \| 2016JGRA..121.4158W \| http://ui.adsabs.harvard.edu/#abs/2016JGRA..121.4158W X-Ray and Optical Followup of Gamma-Ray (up to TeV) Sources \|Masetti, N., \| ChJAS \| 8-124 \| 2008 \| 2008ChJAS...8..124M \| http://ui.adsabs.harvard.edu/#abs/2008ChJAS...8..124M 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 Exospheric Neutral Hydrogen Density at the Nominal 10 RE Subsolar Point Deduced From XMM-Newton X-Ray Observations \|Connor, Hyunju K., Carter, Jennifer A., \| JGRA \| 124-1612 \| 2019 \| 2019JGRA..124.1612C \| http://ui.adsabs.harvard.edu/#abs/2019JGRA..124.1612C 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 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	2001-10-16T04:38:09Z/2002-08-10T15:34:38Z
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	2003-09-06T00:00:00Z
Keywords	"pul sars", "neutron star population", "neutron star cooling", "supernova blast wave", "XMM", "thermal contributions", "pulsars ages", "relativistic wind", "thermal processes", "energetic sources", "thermal physics", "se parate", "xray emission", "contributi ons"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Bryan Gaensler, 2003, 'Disentangling X-ray emission processes in Vela-like pulsars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qv4mb33