A dataset provided by the European Space Agency

Name: Catching magnetar candidates among unidentified INTEGRAL sources with XMM
Published: 2012-03-16T00:00:00Z

Proposal ID	065549
Title	Catching magnetar candidates among unidentified INTEGRAL sources with XMM
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655490101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655490301
DOI	https://doi.org/10.5270/esa-brxa6fe
Principal Investigator, PI	Dr Lucia Pavan
Abstract	Magnetars are a rare class of isolated neutron stars, whose emission propertieschallenged in the past few years all the theories of radiative processes inpresence of extreme magnetic i??elds. Catching new magnetar candidates andenlarge the known sample of these peculiar ob jects is vital in order to testsuch theories, provide the basis for new developments and clarify thedifferences and connections among the whole family of isolated neutron stars.The aim of this proposal is to identify the three most promising magnetarcandidates, selected among a large number of still unidentii??ed INTEGRALsources. Their hard and peculiar X-ray spectrum and closeness to the galacticplane suggested they most likely belong to the magnetar class.
Publications	XMM-Newton observations of four high mass X-ray binaries and IGR J17348-2045 \|Bozzo, E., Pavan, L., et al. \| A&A \| 544-118 \| 2012 \| 2012A&A...544A.118B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...544A.118B Accurate localization and identification of six hard X-ray sources from Chandra and XMM-Newton data \|Karasev, D. I., Lutovinov, A. A., et al. \| AstL \| 38-629 \| 2012 \| 2012AstL...38..629K \| http://ui.adsabs.harvard.edu/#abs/2012AstL...38..629K 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 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	2010-10-16T21:19:56Z/2011-03-02T11:38:45Z
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	2012-03-16T00:00:00Z
Keywords	"rare class", "ed integral sources", "galactic plane suggested", "emission properties challenged", "XMM", "magnetar class", "xray spectrum", "magnetar candidates", "?? elds", "isolated neutron stars", "radiative processes", "promising magnetar candidates", "ob jects", "catching magnetar candidates", "unidentified integral sources"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Lucia Pavan, 2012, 'Catching magnetar candidates among unidentified INTEGRAL sources with XMM', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-brxa6fe