A dataset provided by the European Space Agency

Name: X-Ray Emission from the Halo of M31
Published: 2004-08-02T00:00:00Z

Proposal ID	015158
Title	X-Ray Emission from the Halo of M31
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0151580101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0151580201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0151580301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0151580401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0151581101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0151581201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0151581301
DOI	https://doi.org/10.5270/esa-gha6emb
Principal Investigator, PI	Dr Rosanne Di Stefano
Abstract	We request 100 ksec (net) to study the X-ray properties of the halo of M31. Wepropose to observe 10 halo fields for 10 ksec each, covering 1200 kpc^2. XMMwill detect all point sources with luminosities above virgul10^36 ergs/s; we expectto discover 50-150 M31 halo X-ray sources, including X-ray binaries ejected fromGCs, X-ray binaries ejected from the galaxy.s disk, very hot central stars ofplanetary nebulae, and supersoft X-ray binaries. The fields we have choseninclude 27 globular clusters (GCs), which comprise almost 1/3 of all GCs notprojected onto the the galaxy.s optical disk. These observations will testmodels of galactic halo populations, as well as models for the formation ofX-ray binaries in GCs.
Publications	The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The deep XMM-Newton Survey of M 31 \|Stiele, H., Pietsch, W., et al. \| A&A \| 534-55 \| 2011 \| 2011A&A...534A..55S \| http://ui.adsabs.harvard.edu/#abs/2011A&A...534A..55S An XMM-Newton survey of M 31 \|Pietsch, W., Freyberg, M., \| A&A \| 434-483 \| 2005 \| 2005A&A...434..483P \| http://ui.adsabs.harvard.edu/#abs/2005A&A...434..483P A Close Look at the Population of Supersoft and Quasi-soft X-Ray Sources Observed in M31 with XMM-Newton \|Orio, Marina, \| ApJ \| 643-844 \| 2006 \| 2006ApJ...643..844O \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...643..844O X-Rays from the Globular Cluster G1: Intermediate-Mass Black Hole or Low-Mass X-Ray Binary? \|Pooley, David, Rappaport, Saul, \| ApJ \| 644-45 \| 2006 \| 2006ApJ...644L..45P \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...644L..45P The X-ray source population of the Andromeda galaxy M 31 \|Pietsch, W., \| AN \| 329-170 \| 2008 \| 2008AN....329..170P \| http://ui.adsabs.harvard.edu/#abs/2008AN....329..170P An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 \|Henley, David B., Shelton, Robin L., \| ApJS \| 187-388 \| 2010 \| 2010ApJS..187..388H \| http://ui.adsabs.harvard.edu/#abs/2010ApJS..187..388H A systematic study of low-mass X-ray binaries in the M31 globular cluster system \|Peacock, Mark B., Maccarone, Thomas J., et al. \| MNRAS \| 407-2611 \| 2010 \| 2010MNRAS.407.2611P \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.407.2611P An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C Supernova remnants and candidates detected in the XMM-Newton M 31 large survey \|Sasaki, M., Pietsch, W., et al. \| A&A \| 544-144 \| 2012 \| 2012A&A...544A.144S \| http://ui.adsabs.harvard.edu/#abs/2012A&A...544A.144S Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi, J. A., Albacete Colombo, J. F., et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 The XMM deep survey in the CDF-S. VIII. X-ray properties of the two brightest sources \|Iwasawa, K., Vignali, C., et al. \| A&A \| 574-144 \| 2015 \| 2015A&A...574A.144I \| http://ui.adsabs.harvard.edu/#abs/2015A&A...574A.144I Wide-Field Survey of Globular Clusters in M31. II. Kinematics of the Globular Cluster System \|Lee, Myung Gyoon, Hwang, Ho Seong, et al. \| ApJ \| 674-886 \| 2008 \| 2008ApJ...674..886L \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...674..886L Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X A novel scenario for the possible X-ray line feature at virgul3.5 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 Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 J004457+4123 (Sharov 21): not a remarkable nova in M 31 but a background quasar with a spectacular UV flare \|Meusinger, H., Henze, M., et al. \| A&A \| 512-1 \| 2010 \| 2010A&A...512A...1M \| http://ui.adsabs.harvard.edu/#abs/2010A&A...512A...1M NuSTAR view of the central region of M31 \|Stiele, H., Kong, A. K. H., \| MNRAS \| 475-4911 \| 2018 \| 2018MNRAS.475.4911S \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.4911S 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The 3CR Chandra Snapshot Survey: Extragalactic Radio Sources with Redshifts between 1 and 1.5 \|Stuardi, C., Missaglia, V., et al. \| ApJS \| 235-32 \| 2018 \| 2018ApJS..235...32S \| http://ui.adsabs.harvard.edu/#abs/2018ApJS..235...32S 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 Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals \|Sibeck, David G., Allen, R., et al. \| SSRv \| 214-79 \| 2018 \| 2018SSRv..214...79S \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S 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 The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Comparing Chandra and Hubble in the Northern Disk of M31 \|Williams, Benjamin F., Lazzarini, Margaret, et al. \| ApJS \| 239-13 \| 2018 \| 2018ApJS..239...13W \| http://ui.adsabs.harvard.edu/#abs/2018ApJS..239...13W New constraints on sterile neutrino dark matter from NuSTAR M31 observations \|Ng, Kenny C. Y., Roach, Brandon M., et al. \| PhRvD \| 99-83005 \| 2019 \| 2019PhRvD..99h3005N \| http://ui.adsabs.harvard.edu/#abs/2019PhRvD..99h3005N Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q A Search for the 3.5 keV Line from the Milky Way.s 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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	2002-12-29T05:55:31Z/2003-07-01T16:50:48Z
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	2004-08-02T00:00:00Z
Keywords	"test models", "xray properties", "M31", "globular cluster gcs", "halo fields", "XMM", "xray binary", "x ray emission", "optical disk", "supersoft xray binary", "planetary nebulae", "galactic halo populations", "hot central stars"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Rosanne Di Stefano, 2004, 'X-Ray Emission from the Halo of M31', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gha6emb