A dataset provided by the European Space Agency

Name: X-ray Spectroscopy of the Cumulative Stellar Emission from M32
Published: 2012-08-02T00:00:00Z

Proposal ID	067213
Title	X-ray Spectroscopy of the Cumulative Stellar Emission from M32
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672130101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672130501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672130601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672130701
DOI	https://doi.org/10.5270/esa-hy7q030
Principal Investigator, PI	Prof Q. Daniel Wang
Abstract	We propose a deep XMM-Newton observation of the nearest compact ellipticalgalaxy M32. The RGS will provide the first high-resolution spectrum of thecumulative soft X-ray emission of old stellar populations, with littlecontribution from low-mass X-ray binaries or diffuse hot gas. This spectraltemplate will be useful to the study of the average properties of thepopulations and, most importantly, will facilitate a reliable subtraction of thestellar contribution in the spectroscopic analysis of diffuse hot gas ingalactic spheroids in general. The EPIC spectrum will offer a complementary highsensitivity and broad energy coverage, badly needed for determining the natureof hard X-ray emission observed in the Galactic ridge and in nearby galaxies.
Publications	Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog: Objects of Special Interest \|Lin Dacheng Webb Natalie A. \| ApJ \| 780-39 \| 2014 \| 2014ApJ...780...39L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...780...39L Unidentified Line in X-Ray Spectra of the Andromeda Galaxy and Perseus Galaxy Cluster \|Boyarsky A. Ruchayskiy O. et al. \| PhRvL \| 113-251301 \| 2014 \| 2014PhRvL.113y1301B \| http://ui.adsabs.harvard.edu/#abs/2014PhRvL.113y1301B 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 Detection of a Compact Nuclear Radio Source in the Local Group Elliptical Galaxy M32 \|Yang Yang Li Zhiyuan et al. \| ApJ \| 807-19 \| 2015 \| 2015ApJ...807L..19Y \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...807L..19Y A novel scenario for the possible X-ray line feature at ~3.5 keV. Charge exchange with bare sulfur ions \|Gu L. Kaastra J. et al. \| A&A \| 584-11 \| 2015 \| 2015A&A...584L..11G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...584L..11G 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 X-Ray Lines from Dark Matter Annihilation at the keV Scale \|Brdar Vedran Kopp Joachim et al. \| PhRvL \| 120-61301 \| 2018 \| 2018PhRvL.120f1301B \| http://ui.adsabs.harvard.edu/#abs/2018PhRvL.120f1301B WIMP dark matter candidates and searches---current status and future prospects \|Roszkowski Leszek Sessolo Enrico Maria \| RPPh \| 81-66201 \| 2018 \| 2018RPPh...81f6201R \| http://ui.adsabs.harvard.edu/#abs/2018RPPh...81f6201R Creation of the X-ray sky maps and their application for a search of the dark matter decay line \|Yakubovskyi D. A. Savchenko D. O. \| KosNT \| 21-90 \| 2015 \| 2015KosNT..21e..90Y \| http://ui.adsabs.harvard.edu/#abs/2015KosNT..21e..90Y A new clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw H. P. Roberts T. P. et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E 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 A Search for the 3.5 keV Line from the Milky Ways Dark Matter Halo with HaloSat \|Silich E. M. Jahoda K. et al. \| ApJ \| 916-2 \| 2021 \| 2021ApJ...916....2S \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...916....2S 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 impact of precession on the observed population of ULXs \|Khan Norman Middleton Matthew J. et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows R. Comerford Julia M. et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S 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 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	2011-06-27T06:47:28Z/2011-07-14T16:02:16Z
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	2012-08-02T00:00:00Z
Last Update	2025-01-27
Keywords	"hard xray emission", "broad energy coverage", "nearby galaxy", "diffuse hot gas", "M32", "spectral template", "reliable subtraction", "stellar populations", "galactic spheroids", "resolution spectrum", "average properties", "EPIC", "XMM-Newton", "cumulative stellar emission", "galactic ridge", "epic spectrum", "spectroscopic analysis", "x ray spectroscopy", "XMM", "deep xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Q. Daniel Wang, 2012, 'X-ray Spectroscopy of the Cumulative Stellar Emission from M32', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hy7q030