A dataset provided by the European Space Agency

Name: Dim X-ray Sources in Globular Clusters
Published: 2003-09-04T00:00:00Z

Proposal ID	011222
Title	Dim X-ray Sources in Globular Clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112220101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112220201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0112220301
DOI	https://doi.org/10.5270/esa-lcbdd67
Principal Investigator, PI	Dr Martin Turner
Abstract	GT-We propose to conduct a survey of the globular clusterswith larger cores in which faint sources have been observed byROSAT and EINSTEIN, and use the XMM spectral capabilities todetermine the nature of the dim sources. Characterizing thecontent of globular clusters is of considerable interest fortheories of binary production and evolution, as well as dynamicalevolution and survival of the clusters in which they reside.Question for ngc6656: The integrated V and B of the cluster are 6and 7. Could that be a problem for the OM (magnifier mode)?
Publications	X-ray sources and their optical counterparts in the globular cluster M 22 \|Webb, N. A., Serre, D., et al. \| A&A \| 424-133 \| 2004 \| 2004A&A...424..133W \| http://ui.adsabs.harvard.edu/#abs/2004A&A...424..133W 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 An XMM-Newton observation of the globular cluster Omega Centauri \|Gendre, B., Barret, D., \| A&A \| 400-521 \| 2003 \| 2003A&A...400..521G \| http://ui.adsabs.harvard.edu/#abs/2003A&A...400..521G First XMM-Newton observations of the globular cluster M 22 \|Webb, N. A., Gendre, B., \| A&A \| 381-481 \| 2002 \| 2002A&A...381..481W \| http://ui.adsabs.harvard.edu/#abs/2002A&A...381..481W The XMM-Newton EPIC background: Production of background maps and event files \|Read, A. M., Ponman, T. J., \| A&A \| 409-395 \| 2003 \| 2003A&A...409..395R \| http://ui.adsabs.harvard.edu/#abs/2003A&A...409..395R XMM-Newton data processing for faint diffuse emission. Proton flares, exposure maps and report on EPIC MOS1 bright CCDs contamination \|Pradas, J., Kerp, J., \| A&A \| 443-721 \| 2005 \| 2005A&A...443..721P \| http://ui.adsabs.harvard.edu/#abs/2005A&A...443..721P The XMM-Newton EPIC background and the production of background blank sky event files \|Carter, J. A., Read, A. M., \| A&A \| 464-1155 \| 2007 \| 2007A&A...464.1155C \| http://ui.adsabs.harvard.edu/#abs/2007A&A...464.1155C Constraining the Equation of State of Supranuclear Dense Matter from XMM-Newton Observations of Neutron Stars in Globular Clusters \|Webb, Natalie A., Barret, Didier, \| ApJ \| 671-727 \| 2007 \| 2007ApJ...671..727W \| http://ui.adsabs.harvard.edu/#abs/2007ApJ...671..727W X-ray sources in globular clusters \|Webb, N. A., Gendre, B., \| AN \| 324-147 \| 2003 \| 2003AN....324..147W \| http://ui.adsabs.harvard.edu/#abs/2003AN....324..147W XMM-Newton observations of faint X-ray sources in globular clusters \|Webb, N. A., Barret, D., \| AdSpR \| 38-2930 \| 2006 \| 2006AdSpR..38.2930W \| http://ui.adsabs.harvard.edu/#abs/2006AdSpR..38.2930W 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 Constraints on sterile neutrinos as dark matter candidates from the diffuse X-ray background \|Boyarsky, A., Neronov, A., et al. \| MNRAS \| 370-213 \| 2006 \| 2006MNRAS.370..213B \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.370..213B 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 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca, A., Molendi, S., \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D CV1 in the globular cluster M 22: confirming its nature through X-ray observations and optical spectroscopy \|Webb, N. A., Servillat, M., \| A&A \| 551-60 \| 2013 \| 2013A&A...551A..60W \| http://ui.adsabs.harvard.edu/#abs/2013A&A...551A..60W Statistical Properties of Galactic delta Scuti Stars: Revisited \|Chang, S.-W., Protopapas, P., et al. \| AJ \| 145-132 \| 2013 \| 2013AJ....145..132C \| http://ui.adsabs.harvard.edu/#abs/2013AJ....145..132C Measurement of the Radius of Neutron Stars with High Signal-to-noise Quiescent Low-mass X-Ray Binaries in Globular Clusters \|Guillot, Sebastien, Servillat, Mathieu, et al. \| ApJ \| 772-7 \| 2013 \| 2013ApJ...772....7G \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...772....7G Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L Improved mass and radius constraints for quiescent neutron stars in omega Cen and NGC 6397 \|Heinke, C. O., Cohn, H. N., et al. \| MNRAS \| 444-443 \| 2014 \| 2014MNRAS.444..443H \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444..443H 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 Rejecting Proposed Dense Matter Equations of State with Quiescent Low-mass X-Ray Binaries \|Guillot, Sebastien, Rutledge, Robert E., \| ApJ \| 796-3 \| 2014 \| 2014ApJ...796L...3G \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...796L...3G Cluster AgeS Experiment (CASE): Dwarf Novae and a Probable Microlensing Event in the Globular Cluster M22 \|Pietrukowicz, P., Kaluzny, J., et al. \| AcA \| 55-261 \| 2005 \| 2005AcA....55..261P \| http://ui.adsabs.harvard.edu/#abs/2005AcA....55..261P 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 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 Chandra Detections of Diffuse X-Ray Emission from Globular Clusters \|Okada, Yuu, Kokubun, Motohide, et al. \| PASJ \| 59-727 \| 2007 \| 2007PASJ...59..727O \| http://ui.adsabs.harvard.edu/#abs/2007PASJ...59..727O 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 Constraining the mass and radius of neutron stars in globular clusters \|Steiner, A. W., Heinke, C. O., et al. \| MNRAS \| 476-421 \| 2018 \| 2018MNRAS.476..421S \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.476..421S 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 The Spectrum of the Universe \|Hill, Ryley, Masui, Kiyoshi W., \| ApSpe \| 72-663 \| 2018 \| 2018ApSpe..72..663H \| http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H A Deep X-ray Survey of the globular cluster Omega Centauri \|Henleywillis, Simon, Cool, Adrienne M., et al. \| MNRAS \| 479-2834 \| 2018 \| 2018MNRAS.479.2834H \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.479.2834H Search for multiwavelength emission from the binary millisecond pulsar PSR J1836-2354A in the globular cluster M22 \|Amato, R., D.Ai, A., et al. \| MNRAS \| 486-3992 \| 2019 \| 2019MNRAS.486.3992A \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.486.3992A 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 Discovery of Millisecond Pulsars in the Globular Cluster Omega Centauri \|Dai, Shi, Johnston, Simon, et al. \| ApJ \| 888-18 \| 2020 \| 2020ApJ...888L..18D \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...888L..18D New Constraints on the Nuclear Equation of State from the Thermal Emission of Neutron Stars in Quiescent Low-mass X-Ray Binaries \|Baillot d\\u2019Etivaux, Nicolas, Guillot, Sebastien, et al. \| ApJ \| 887-48 \| 2019 \| 2019ApJ...887...48B \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...887...48B 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 Decaying fermionic warm dark matter and XENON1T electronic recoil excess \|Dutta, Koushik, Ghosh, Avirup, et al. \| PDU \| 33-100855 \| 2021 \| 2021PDU....3300855D \| http://ui.adsabs.harvard.edu/#abs/2021PDU....3300855D 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 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 Properties of Milky Way globular clusters associated with X-ray sources \|Botev, Svetoslav, Nedialkov, Petko, \| BlgAJ \| 40-59 \| 2024 \| 2024BlgAJ..40...59B \| http://ui.adsabs.harvard.edu/#abs/2024BlgAJ..40...59B 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	2000-09-19T22:05:00Z/2001-08-13T10:50:51Z
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	2003-09-04T00:00:00Z
Keywords	"XMM", "dim sources", "dim xray sources", "globular clusters", "binary production", "dynamical evolution", "om magnifier mode", "globular cluster", "faint sources", "larger cores", "ROSAT", "xmm spectral"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Martin Turner, 2003, 'Dim X-ray Sources in Globular Clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-lcbdd67