A dataset provided by the European Space Agency

Name: Deep observations of the northern disc of M31
Published: 2017-02-05T23:00:00Z

Proposal ID	076312
Title	Deep observations of the northern disc of M31
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763120101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763120201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763120301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763120401
DOI	https://doi.org/10.5270/esa-rouvsy2
Principal Investigator, PI	Dr Manami Sasaki
Abstract	The XMM-Newton survey of M31 has revealed extended diffuse emission, inparticular on the northern side, which is well correlated with the northernstar-forming ring of the galaxy. We propose two deep pointings with 200 ksexposure each to cover the star-forming disc and to perform a detailed study ofthe diffuse emission. We will thus map the X-ray emission of the hotinterstellar medium (ISM) in a spiral galaxy like our own on arcmin scales andmeasure the temperature, density, and filling factor of brighter ISM structures.In addition, we will obtain a complete list of X-ray sources in the northerndisc of M31 down to the confusion limit of a few 10^34 erg s^-1, with improvedvariability and spectral information for all sources.
Publications	Deep XMM-Newton observations of the northern disc of M 31. I. Source catalogue \|Sasaki Manami Haberl Frank et al. \| A&A \| 620-28 \| 2018 \| 2018A&A...620A..28S \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A..28S A recurrent nova super-remnant in the Andromeda galaxy \|Darnley M. J. Hounsell R. et al. \| Natur \| 565-460 \| 2019 \| 2019Natur.565..460D \| http://ui.adsabs.harvard.edu/#abs/2019Natur.565..460D Deep XMM-Newton observations of the northern disc of M31. II. Tracing the hot interstellar medium \|Kavanagh Patrick J. Sasaki Manami et al. \| A&A \| 637-12 \| 2020 \| 2020A&A...637A..12K \| http://ui.adsabs.harvard.edu/#abs/2020A&A...637A..12K Multiwavelength Characterization of the High-mass X-Ray Binary Population of M31 \|Lazzarini Margaret Williams Benjamin F. et al. \| ApJ \| 906-120 \| 2021 \| 2021ApJ...906..120L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...906..120L 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 On the observability of recurrent nova super-remnants \|Healy-Kalesh M. W. Darnley M. J. et al. \| MNRAS \| 521-3004 \| 2023 \| 2023MNRAS.521.3004H \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.521.3004H An XMM-Newton View of the Andromeda Galaxy as Explored in a Legacy Survey (New-ANGELS). I. The X-Ray Source Catalog \|Huang Rui Li Jiang-Tao et al. \| ApJS \| 268-36 \| 2023 \| 2023ApJS..268...36H \| http://ui.adsabs.harvard.edu/#abs/2023ApJS..268...36H 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	2015-06-28T06:07:53Z/2016-01-22T23:08:07Z
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	2017-02-05T23:00:00Z
Last Update	2025-01-27
Keywords	"arcmin scales", "M31", "complete list", "spiral galaxy", "improved variability", "northern disc", "brighter ism structures", "XMM-Newton", "deep pointings", "star forming disc", "spectral information", "xray emission", "xray sources", "filling factor", "XMM", "diffuse emission", "confusion limit", "xmm newton survey"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Manami Sasaki, 2017, 'Deep observations of the northern disc of M31', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rouvsy2