A dataset provided by the European Space Agency

Name: Search for the roots of the Cygnus Loop
Published: 2005-01-01T00:00:00Z

Proposal ID	008254
Title	Search for the roots of the Cygnus Loop
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0082540101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0082540201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0082540301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0082540401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0082540501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0082540601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0082540701
DOI	https://doi.org/10.5270/esa-drf7rbq
Principal Investigator, PI	Dr Emi Miyata
Abstract	We propose to observe the Cygnus Loop to investigate the progenitor starand study its roots. Basedon the ASCA observation, we found that there was a metal rich plasmaleft in the core of the Loop. It must be a fossil of the supernovaexplosion. The relative abundance ratio suggested that the CygnusLoop originated from the 25 Msun star expecting the production of acompact star. The scientific goal of the observation is to study thefossil: what the structure of the fossil is, how it is mixing with theISM, what makes an asymmetry.
Publications	Line-of-Sight Shell Structure of the Cygnus Loop \|Uchida Hiroyuki Tsunemi Hiroshi et al. \| ApJ \| 705-1152 \| 2009 \| 2009ApJ...705.1152U \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...705.1152U 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 Plasma Structure of the Cygnus Loop from the Northeastern Rim to the Southwestern Rim \|Tsunemi Hiroshi Katsuda Satoru et al. \| ApJ \| 671-1717 \| 2007 \| 2007ApJ...671.1717T \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...671.1717T XMM-Newton Observation of the Northeastern Limb of the Cygnus Loop \|Nemes Norbert Tsunemi Hiroshi \| ApJ \| 675-1293 \| 2008 \| 2008ApJ...675.1293N \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...675.1293N XMM-Newton observations across the Cygnus Loop from northeastern rim to southwestern rim \|Katsuda Satoru Tsunemi Hiroshi \| AdSpR \| 41-383 \| 2008 \| 2008AdSpR..41..383K \| http://ui.adsabs.harvard.edu/#abs/2008AdSpR..41..383K First Detection of Ar-K Line Emission from the Cygnus Loop \|Uchida Hiroyuki Tsunemi Hiroshi et al. \| PASJ \| 63-199 \| 2011 \| 2011PASJ...63..199U \| http://ui.adsabs.harvard.edu/#abs/2011PASJ...63..199U 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 Joint Suzaku and XMM-Newton Spectral Analysis of the Southwest Cygnus Loop \|Leahy Denis Hassan Mohammed \| ApJ \| 764-55 \| 2013 \| 2013ApJ...764...55L \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...764...55L 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 The Chandra ACIS Timing Survey Project: glimpsing a sample of faint X-ray pulsators \|Israel G. L. Esposito P. et al. \| MNRAS \| 462-4371 \| 2016 \| 2016MNRAS.462.4371I \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.462.4371I 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 Ejecta Distributions of Heavy Elements in the Cygnus Loop \|Uchida Hiroyuki Tsunemi Hiroshi et al. \| PASJ \| 61-301 \| 2009 \| 2009PASJ...61..301U \| http://ui.adsabs.harvard.edu/#abs/2009PASJ...61..301U 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	2002-11-25T22:55:01Z/2002-12-14T01:53:06Z
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	2005-01-01T00:00:00Z
Last Update	2025-01-27
Keywords	"progenitor star", "supernova explosion", "compact star", "msun star expecting", "cygnus loop", "cygnus loop originated"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Emi Miyata, 2005, 'Search for the roots of the Cygnus Loop', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-drf7rbq