A dataset provided by the European Space Agency

Name: Imaging G75.2+0.1 comma the Pulsar Wind Nebula of a Likely Gamma-ray Pulsar
Published: 2007-06-13T00:00:00Z

Proposal ID	040454
Title	Imaging G75.2+0.1, the Pulsar Wind Nebula of a Likely Gamma-ray Pulsar
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0404540101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0404540201
DOI	https://doi.org/10.5270/esa-qgieogt
Principal Investigator, PI	Dr Mallory Roberts
Abstract	We propose a 75-ks observation with XMM-Newton to study the recently-discoveredpulsar wind nebula G75.2+0.1, which is associated with the Vela-like pulsar PSRJ2021+3651. These observations will complement a 19.0-ks Chandra observation ofthe source made by our group, which discovered thermal X-rays from the pulsar aswell as an apparently toroidal inner nebula. XMM.s larger effective area andfield of view will allow us to image and perform spectroscopy on the faintdiffuse emission surrounding the inner nebula, and to determine whether faintjets, hinted at by our Chandra observation, are indeed present along thenebula.s axis of symmetry.
Publications	X-rays from colliding stellar winds: the case of close Wolf-Rayet+O binary systems \|Zhekov, Svetozar A., \| MNRAS \| 422-1332 \| 2012 \| 2012MNRAS.422.1332Z \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.422.1332Z 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 X-Ray and Gamma-Ray Observations of the Inner Region of Mgro J2019+37 \|Zabalza, V., Paredes, J. M., \| IJMPD \| 19-811 \| 2010 \| 2010IJMPD..19..811Z \| http://ui.adsabs.harvard.edu/#abs/2010IJMPD..19..811Z 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 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 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 Spatially Resolving the Very High Energy Emission from MGRO J2019+37 with VERITAS \|Aliu, E., Aune, T., et al. \| ApJ \| 788-78 \| 2014 \| 2014ApJ...788...78A \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...788...78A 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 Synchrotron emission model of gamma-ray pulsar PSR J2021+3651 \|Chkheidze, N., Babyk, Iu., \| NewA \| 35-27 \| 2015 \| 2015NewA...35...27C \| http://ui.adsabs.harvard.edu/#abs/2015NewA...35...27C Radio continuum and near-infrared study of the MGRO J2019+37 region \|Paredes, J. M., Marti, J., et al. \| A&A \| 507-241 \| 2009 \| 2009A&A...507..241P \| http://ui.adsabs.harvard.edu/#abs/2009A&A...507..241P 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 Multi-wavelength study of MGRO J2019+37 \|Hou, Chao, Chen, Song-Zhan, et al. \| ChPhC \| 38-85001 \| 2014 \| 2014ChPhC..38h5001H \| http://ui.adsabs.harvard.edu/#abs/2014ChPhC..38h5001H 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 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 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	2006-05-19T10:39:36Z/2006-05-21T20:11:46Z
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	2007-06-13T00:00:00Z
Keywords	"thermal xray", "inner nebula", "imaging g75", "XMM", "G75.2", "larger effective", "gamma ray pulsar", "faint diffuse emission", "faint jets", "pulsar psr j2021", "XMM-Newton", "perform spectroscopy", "pulsar wind nebula", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Mallory Roberts, 2007, 'Imaging G75.2+0.1 comma the Pulsar Wind Nebula of a Likely Gamma-ray Pulsar', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-qgieogt