A dataset provided by the European Space Agency

Name: WR 47 comma a binary harbouring a massive late WN comma and the faint open cluster Hogg 15
Published: 2004-02-21T00:00:00Z

Proposal ID	010948
Title	WR 47, a binary harbouring a massive late WN, and the faint open cluster Hogg 15
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109480101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109480201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109480401
DOI	https://doi.org/10.5270/esa-1mfu10e
Principal Investigator, PI	Prof Mason Keith
Abstract	GT- The spectral characteristics of the Wolf Rayet starWR 47 will be obtained at different binary phases. Although not flagged as a fixed observation, these observationsneed to be made at particular binary phases. The attached postscript file lists these time constraintsthat were not possible to include in the fixed observation section.
Publications	X-ray emission characteristics of two Wolf-Rayet binaries: V444 Cyg and CD Cru \|Bhatt, Himali, Pandey, J. C., et al. \| MNRAS \| 402-1767 \| 2010 \| 2010MNRAS.402.1767B \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.402.1767B 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 X-rays from colliding stellar winds: the case of close Wolf-Rayet+O binary systems \|Zhekov, Svetozar A., \| MNRAS \| 422-1332 \| 2012 \| 2012MNRAS.422.1332Z \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.422.1332Z 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 On the X-ray and optical properties of the Be star HD 110432: a very hard-thermal X-ray emitter \|Lopes de Oliveira, R., Motch, C., et al. \| A&A \| 474-983 \| 2007 \| 2007A&A...474..983L \| http://ui.adsabs.harvard.edu/#abs/2007A&A...474..983L A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations \|Muno, M. P., Gaensler, B. M., et al. \| ApJ \| 680-639 \| 2008 \| 2008ApJ...680..639M \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...680..639M 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 Characterization of the X-Ray Light Curve of the gamma Cas-like B1e Star HD 110432 \|Smith, Myron A., Lopes de Oliveira, Raimundo, \| ApJ \| 755-64 \| 2012 \| 2012ApJ...755...64S \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...755...64S 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 Hot stars observed by XMM-Newton. I. The catalog and the properties of OB stars \|Naze, Y., \| A&A \| 506-1055 \| 2009 \| 2009A&A...506.1055N \| http://ui.adsabs.harvard.edu/#abs/2009A&A...506.1055N 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 X-ray Observations of Eight Young Open Star Clusters: I. Membership and X-ray Luminosity \|Bhatt, Himali, Pandey, J. C., et al. \| JApA \| 34-393 \| 2013 \| 2013JApA...34..393B \| http://ui.adsabs.harvard.edu/#abs/2013JApA...34..393B 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 Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra \|Nunez, N. E., Luna, G. J. M., et al. \| A&A \| 565-82 \| 2014 \| 2014A&A...565A..82N \| http://ui.adsabs.harvard.edu/#abs/2014A&A...565A..82N 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 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 Deteccion de la estrella simbiotica Hen 2-87 en rayos X con XMM-Newton \|Nunnez, N. E., Luna, G. J. M., \| BAAA \| 55-491 \| 2012 \| 2012BAAA...55..491N \| http://ui.adsabs.harvard.edu/#abs/2012BAAA...55..491N 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 Hot stars observed by XMM-Newton. II. A survey of Oe and Be stars \|Naze, Yael, Motch, Christian, \| A&A \| 619-148 \| 2018 \| 2018A&A...619A.148N \| http://ui.adsabs.harvard.edu/#abs/2018A&A...619A.148N 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 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 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	2002-07-03T14:59:24Z/2003-01-21T13:35:45Z
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	2004-02-21T00:00:00Z
Keywords	"binary phases", "file lists", "spectral characteristics", "massive late wn", "time constraints", "cluster hogg", "binary harbouring"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Mason Keith, 2004, 'WR 47 comma a binary harbouring a massive late WN comma and the faint open cluster Hogg 15', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-1mfu10e