A dataset provided by the European Space Agency

Name: Identification campaign of supernova remnant candidates in the Milky Way
Published: 2014-05-30T00:00:00Z

Proposal ID	072344
Title	Identification campaign of supernova remnant candidates in the Milky Way
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723440101
DOI	https://doi.org/10.5270/esa-e786q3f
Principal Investigator, PI	Dr Regina H. H. Huang
Abstract	There are 302 supernova remnants (SNRs) have been identified in the Milky Way.Most SNRs are discovered in radio surveys. In view of various selection effects,the current sample of SNRs is clearly incomplete. ROSAT all-sky survey data haveprovided another window to search for SNRs. We have chosen some bright andpromising SNR candidates as the starting point of a long-term identificationcampaign. We propose a set of short XMM-Newton observations to have a fullcoverage of these targets in order to investigate their spectra and morphologiesin details as well as to search for the associated compact stellar remnantsproduced in the supernova explosions.
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 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	2013-05-20T10:43:02Z/2013-05-20T17:16:28Z
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	2014-05-30T00:00:00Z
Keywords	"short xmm newton", "identification campaign", "sky survey data", "XMM", "supernova remnant", "supernova explosions", "selection effects", "compact stellar remnant", "XMM-Newton", "term identification campaign", "supernova remnant candidates", "ROSAT", "radio surveys"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Regina H. H. Huang, 2014, 'Identification campaign of supernova remnant candidates in the Milky Way', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-e786q3f