A dataset provided by the European Space Agency

Name: Unveiling the X-ray Properties of the PWN G63.7+1.1 with XMM-Newton
Published: 2010-05-22T00:00:00Z

Proposal ID	060338
Title	Unveiling the X-ray Properties of the PWN G63.7+1.1 with XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0603380101
DOI	https://doi.org/10.5270/esa-96mn6wv
Principal Investigator, PI	Prof Samar Safi-Harb
Abstract	PWNe offer a valuable astrophysical laboratory to study the physics of pulsaroutflows and their interaction with their surrounding medium. Their X-ray studyin particular offers insights into the energetics of the powering engine, thecharacteristics of the pulsar wind, and the conditions of the confining ambientmedium. We propose a 70ks XMM-Newton observation of G63.7+1.1, a PWN discoveredat radio wavelengths, but not yet explored in X-rays. Our proposed study, whencorrelated with our radio data obtained with the CGPS and the Effelsberg radiotelescope, and with new CO data acquired with the JCMT, should allow us toanswer many of the unknown yet basic properties of this object, including itsdistance, age, magnetic field geometry and strength, and the energetics of its powering engine.
Publications	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 XMM-Newton and Chandra Observations of the Filled-center Supernova Remnant G63.7+1.1 \|Matheson H. Safi-Harb S. \| ApJ \| 825-134 \| 2016 \| 2016ApJ...825..134M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...825..134M 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 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	2009-05-04T10:17:26Z/2009-05-05T08:27:40Z
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	2010-05-22T00:00:00Z
Last Update	2025-01-27
Keywords	"pulsar wind", "basic properties", "radio wavelengths", "confining ambient medium", "co data", "magnetic field geometry", "xmm newton", "effelsberg radio telescope", "XMM-Newton", "pulsar outflows", "xray properties", "pwn g63", "powering engine", "G63.7", "XMM", "valuable astrophysical laboratory", "radio data"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Samar Safi-Harb, 2010, 'Unveiling the X-ray Properties of the PWN G63.7+1.1 with XMM-Newton', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-96mn6wv