A dataset provided by the European Space Agency

Name: Exploring the Wing of the SMC
Published: 2017-12-22T23:00:00Z

Proposal ID	078469
Title	Exploring the Wing of the SMC
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784690101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784690201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784690301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784690401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784690601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784690701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784690801
DOI	https://doi.org/10.5270/esa-dok8bgr
Principal Investigator, PI	Dr Frank Haberl
Abstract	The Magellanic Cloud provides the nearest example for tidally interacting andstar-forming galaxies. The wing of the Small Magellanic Cloud is an excellenttarget, to study sources in a tidally disturbed environment. We propose tosurvey further regions of the wing of the Small Magellanic Cloud to betterconstrain the X-ray source population and the amount of diffuse X-ray emissionin this region.
Publications	Identification of AGN in the XMM-Newton X-ray survey of the SMC \|Maitra Chandreyee Haberl Frank et al. \| A&A \| 622-29 \| 2019 \| 2019A&A...622A..29M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...622A..29M 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 SRG/eROSITA discovery of 164 s pulsations from the SMC Be/X-ray binary XMMU J010429.4-723136 \|Carpano S. Haberl F. et al. \| A&A \| 661-20 \| 2022 \| 2022A&A...661A..20C \| http://ui.adsabs.harvard.edu/#abs/2022A&A...661A..20C 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	2016-04-30T17:36:42Z/2016-12-10T23:31:09Z
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	2017-12-22T23:00:00Z
Last Update	2025-01-27
Keywords	"magellanic cloud", "tidally interacting", "diffuse xray emission", "xray source population", "star forming galaxy", "tidally disturbed"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Frank Haberl, 2017, 'Exploring the Wing of the SMC', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-dok8bgr