A dataset provided by the European Space Agency

Name: XMM-Newton observations of three newly discovered supernova remnants
Published: 2015-11-26T23:00:00Z

Proposal ID	074517
Title	XMM-Newton observations of three newly discovered supernova remnants
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745170101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745170201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745170301
DOI	https://doi.org/10.5270/esa-j8ycmnh
Principal Investigator, PI	Mr Tobias Prinz
Abstract	We propose XMM-Newton observations of three newly discovered supernova remnants.With the data we will be able to explore these objects in detail in the X-rayregime. We can measure their spectral characteristics (e.g., temperature,abundance), pinpoint details of their morphology and determine their expansionvelocity as well as estimate their age and distance. The proposed targetsG64.0--0.1 and G83.2+6.9 show radio shells. The southern target G312.4+4.8 has amatch both in the infrared and optical regime. By analyzing the three sources atthese wavelengths we were able to identify them as supernova remnants. Therequested XMM-Newton data will therefore be of high r^ance to complement theobservations, which we performed at other wavelengths.
Publications	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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2014-03-06T07:15:28Z/2014-11-08T04:59:38Z
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	2015-11-26T23:00:00Z
Last Update	2025-01-27
Keywords	"spectral characteristics", " temperature", "xray regime", "xmm newton", "southern target g312", "targets g64", "supernova remnant", "XMM-Newton", "G64.0", "radio shells", "expansion velocity", ".", "optical regime", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Tobias Prinz, 2015, 'XMM-Newton observations of three newly discovered supernova remnants', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-j8ycmnh