A dataset provided by the European Space Agency

Name: The X-ray source populations of different stellar generations in the SMC
Published: 2009-04-03T00:00:00Z

Proposal ID	050300
Title	The X-ray source populations of different stellar generations in the SMC
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503000201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0503000301
DOI	https://doi.org/10.5270/esa-cp0elgb
Principal Investigator, PI	Dr Andreas Zezas
Abstract	We propose XMM-Newton observations of 3 fields of the Small Magellanic Cloud(SMC) with stellar populations virgul100-500 Myr old. These observations were part ofan AO4 program to study the X-ray Binaries (XRBs) of 10 to 500 Myr old stellarpopulations down to Lxvirgul2.5e33 erg/s. Two young fields were successfullyobserved, while the proposed (older) fields were affected by radiation or notobserved. Based on X-ray spectra and timing analysis we will identify X-raybinary pulsars down to spin periods less than 10s. With these results we willstudy the connection between stellar and XRB populations and complement Chandraand XMM-Newton observations of the SMC and other galaxies where faint XRBscannot be observed.
Publications	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 New XMM-Newton observations of supernova remnants in the Small Magellanic Cloud \|Filipovic, M. D., Haberl, F., et al. \| A&A \| 485-63 \| 2008 \| 2008A&A...485...63F \| http://ui.adsabs.harvard.edu/#abs/2008A&A...485...63F Star Formation History and X-ray Binary Populations: The Case of the Small Magellanic Cloud \|Antoniou, V., Zezas, A., et al. \| ApJ \| 716-140 \| 2010 \| 2010ApJ...716L.140A \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...716L.140A An XMM-Newton view of planetary nebulae in the Small Magellanic Cloud. The X-ray luminous central star of SMP SMC 22 \|Mereghetti, S., Krachmalnicoff, N., et al. \| A&A \| 519-42 \| 2010 \| 2010A&A...519A..42M \| http://ui.adsabs.harvard.edu/#abs/2010A&A...519A..42M The XMM-Newton survey of the Small Magellanic Cloud: a new X-ray view of the symbiotic binary SMC 3 \|Sturm, R., Haberl, F., et al. \| A&A \| 529-152 \| 2011 \| 2011A&A...529A.152S \| http://ui.adsabs.harvard.edu/#abs/2011A&A...529A.152S Highly absorbed X-ray binaries in the Small Magellanic Cloud \|Novara, G., La Palombara, N., et al. \| A&A \| 532-153 \| 2011 \| 2011A&A...532A.153N \| http://ui.adsabs.harvard.edu/#abs/2011A&A...532A.153N 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 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 The XMM-Newton survey of the Small Magellanic Cloud \|Haberl, F., Sturm, R., et al. \| A&A \| 545-128 \| 2012 \| 2012A&A...545A.128H \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A.128H 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 survey of the Small Magellanic Cloud: The X-ray point-source catalogue \|Sturm, R., Haberl, F., et al. \| A&A \| 558-3 \| 2013 \| 2013A&A...558A...3S \| http://ui.adsabs.harvard.edu/#abs/2013A&A...558A...3S Active galactic nuclei behind the SMC selected from radio and X-ray surveys \|Sturm, R., Draskovic, D., et al. \| A&A \| 558-101 \| 2013 \| 2013A&A...558A.101S \| http://ui.adsabs.harvard.edu/#abs/2013A&A...558A.101S 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 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 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 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 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 A Comprehensive Library of X-Ray Pulsars in the Small Magellanic Cloud: Time Evolution of Their Luminosities and Spin Periods \|Yang, J., Laycock, S. G. T., et al. \| ApJ \| 839-119 \| 2017 \| 2017ApJ...839..119Y \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...839..119Y SXP 15.6: X-ray spectral and temporal properties of a newly discovered pulsar in the Small Magellanic Cloud \|Vasilopoulos, G., Zezas, A., et al. \| MNRAS \| 470-4354 \| 2017 \| 2017MNRAS.470.4354V \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470.4354V 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 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 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 New optically identified supernova remnants in the Large Magellanic Cloud \|Yew, Miranda, Filipovi\\u0107, Miroslav D., et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y 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 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 Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud \|Matsuura, Mikako, Ayley, Victoria, et al. \| MNRAS \| 513-1154 \| 2022 \| 2022MNRAS.513.1154M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.1154M The MeerKAT 1.3 GHz Survey of the Small Magellanic Cloud \|Cotton, W. D., Filipovi\\u0107, M. D., et al. \| MNRAS \| 529-2443 \| 2024 \| 2024MNRAS.529.2443C \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.2443C 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	2007-10-28T05:49:16Z/2008-03-17T00:04:49Z
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	2009-04-03T00:00:00Z
Keywords	"ao4 program", "xray binary pulsars", "XMM", "faint xrbs", "xrb populations", "spin periods", "xray binary xrbs", "magellanic cloud smc", "5e33 erg", "XMM-Newton", "complement chandra", "xray source populations", "xray spectra", "stellar populations", "stellar generations", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Andreas Zezas, 2009, 'The X-ray source populations of different stellar generations in the SMC', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-cp0elgb