A dataset provided by the European Space Agency

Name: An XMM-Newton Survey of Rich Open Clusters
Published: 2009-11-15T00:00:00Z

Proposal ID	055351
Title	An XMM-Newton Survey of Rich Open Clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553510901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553511001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553511201 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0553511301
DOI	https://doi.org/10.5270/esa-rercq3l
Principal Investigator, PI	Dr David Pooley
Abstract	We know from observations that globular clusters are efficient catalysts informing unusual close binary systems and their offspring, and we seek to explorethis phenomenon in rich open clusters. We propose a uniform survey of 8 nearbyclusters spanning a range of ages and metallicities. The large field of view,high sensitivity, and spatial resolution of XMM are well-matched to such asurvey. Similar studies of globulars, undertaken by us, have revealed a linkbetween a cluster.s internal dynamics and its population of X-ray sources. Wewill examine this link in a regime of stellar density and encounter frequencythat is only accessible via the study of open clusters. In addition, UV andU-band photometry will be invaluable to our ongoing studies of open cluster binaries.
Publications	An Unexpected Discovery in the Rich Open Cluster NGC 6819 Using XMM-Newton \|Gosnell, Natalie M., Pooley, David, et al. \| ApJ \| 745-57 \| 2012 \| 2012ApJ...745...57G \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...745...57G Estimation of the XUV radiation onto close planets and their evaporation \|Sanz-Forcada, J., Micela, G., et al. \| A&A \| 532-6 \| 2011 \| 2011A&A...532A...6S \| http://ui.adsabs.harvard.edu/#abs/2011A&A...532A...6S 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 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 Kepler observations of flaring in A-F type stars \|Balona, L. A., \| MNRAS \| 423-3420 \| 2012 \| 2012MNRAS.423.3420B \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3420B X-ray emission regimes and rotation sequences in M 35 . An updated model of stellar activity evolution on the main sequence \|Gondoin, P., \| A&A \| 556-14 \| 2013 \| 2013A&A...556A..14G \| http://ui.adsabs.harvard.edu/#abs/2013A&A...556A..14G 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 WIYN Open Cluster Study. LXVI. Spectroscopic Binary Orbits in the Young Open Cluster M35 (NGC 2168) \|Leiner, E. M., Mathieu, R. D., et al. \| AJ \| 150-10 \| 2015 \| 2015AJ....150...10L \| http://ui.adsabs.harvard.edu/#abs/2015AJ....150...10L 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 Activity and rotation of the X-ray emitting Kepler stars \|Pizzocaro, D., Stelzer, B., et al. \| A&A \| 628-41 \| 2019 \| 2019A&A...628A..41P \| http://ui.adsabs.harvard.edu/#abs/2019A&A...628A..41P The X-ray emissivity of low-density stellar populations \|Heinke, C. O., Ivanov, M. G., et al. \| MNRAS \| 492-5684 \| 2020 \| 2020MNRAS.492.5684H \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.492.5684H 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 EXTraS project: Exploring the X-ray transient and variable sky \|De Luca, A., Salvaterra, R., et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D 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 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	2008-05-05T15:42:04Z/2008-10-15T07:39:53Z
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	2009-11-15T00:00:00Z
Keywords	"uniform survey", "xray sources", "XMM", "nearby cluster spanning", "accessible via", "close binary systems", "encounter frequency", "xmm newton survey", "efficient catalysts", "globular cluster", "stellar density", "band photometry", "XMM-Newton", "spatial resolution", "cluster binary", "internal dynamics"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr David Pooley, 2009, 'An XMM-Newton Survey of Rich Open Clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rercq3l