A dataset provided by the European Space Agency

Name: MOS soft response and Contamination Monitoring
Published: 2003-10-28T00:00:00Z

Proposal ID	016196
Title	MOS soft response and Contamination Monitoring
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0161960201
DOI	https://doi.org/10.5270/esa-bll92jp
Principal Investigator, PI	Mr Fred Jansen XMM-Newton PS
Abstract	see NRCO #25
Publications	Long-term variability in the X-ray emission of RX J0720.4-3125 \|de Vries, C. P., Vink, J., et al. \| A&A \| 415-31 \| 2004 \| 2004A&A...415L..31D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...415L..31D Evidence for precession of the isolated neutron star RX J0720.4-3125 \|Haberl, F., Turolla, R., et al. \| A&A \| 451-17 \| 2006 \| 2006A&A...451L..17H \| http://ui.adsabs.harvard.edu/#abs/2006A&A...451L..17H A self-consistent model of isolated neutron stars: the case of the X-ray pulsar RX J0720.4-3125 \|Perez-Azorin, J. F., Pons, J. A., et al. \| A&A \| 459-175 \| 2006 \| 2006A&A...459..175P \| http://ui.adsabs.harvard.edu/#abs/2006A&A...459..175P XMM-Newton RGS spectrum of RX J0720.4-3125: an absorption feature at 0.57 keV \|Hambaryan, V., Neuhauser, R., et al. \| A&A \| 497-9 \| 2009 \| 2009A&A...497L...9H \| http://ui.adsabs.harvard.edu/#abs/2009A&A...497L...9H Updated phase coherent timing solution of the isolated neutron star RX J0720.4-3125 using recent XMM-Newton and Chandra observations \|Hohle, M. M., Haberl, F., et al. \| A&A \| 521-11 \| 2010 \| 2010A&A...521A..11H \| http://ui.adsabs.harvard.edu/#abs/2010A&A...521A..11H Narrow absorption features in the co-added XMM-Newton RGS spectra of isolated neutron stars \|Hohle, M. M., Haberl, F., et al. \| MNRAS \| 419-1525 \| 2012 \| 2012MNRAS.419.1525H \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.419.1525H The continued spectral and temporal evolution of RX J0720.4-3125 \|Hohle, M. M., Haberl, F., et al. \| MNRAS \| 423-1194 \| 2012 \| 2012MNRAS.423.1194H \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1194H Spectral and temporal variations of the isolated neutron star RX J0720.4-3125: new XMM-Newton observations \|Hohle, M. M., Haberl, F., et al. \| A&A \| 498-811 \| 2009 \| 2009A&A...498..811H \| http://ui.adsabs.harvard.edu/#abs/2009A&A...498..811H The Continued Spectral Evolution of the Neutron Star RX J0720.4-3125 \|Vink, Jacco, de Vries, Cor P., et al. \| ApJ \| 609-75 \| 2004 \| 2004ApJ...609L..75V \| http://ui.adsabs.harvard.edu/#abs/2004ApJ...609L..75V A Coherent Timing Solution for the Nearby Isolated Neutron Star RX J0720.4-3125 \|Kaplan, D. L., van Kerkwijk, M. H., \| ApJ \| 628-45 \| 2005 \| 2005ApJ...628L..45K \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...628L..45K Thermal emission from isolated neutron stars and their surface magnetic field: Going quadrupolar? \|Zane, S., Turolla, R., \| AdSpR \| 35-1162 \| 2005 \| 2005AdSpR..35.1162Z \| http://ui.adsabs.harvard.edu/#abs/2005AdSpR..35.1162Z Unveiling the thermal and magnetic map of neutron star surfaces though their X-ray emission: method and light-curve analysis \|Zane, Silvia, Turolla, Roberto, \| MNRAS \| 366-727 \| 2006 \| 2006MNRAS.366..727Z \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.366..727Z Towards self-consistent models of isolated neutron stars \|Pons, J. A., Perez-Azorin, J. F., et al. \| Ap&SS \| 308-247 \| 2007 \| 2007Ap&SS.308..247P \| http://ui.adsabs.harvard.edu/#abs/2007Ap&SS.308..247P 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 Discovery of a Strongly Phase-variable Spectral Feature in the Isolated Neutron Star RX J0720.4-3125 \|Borghese, A., Rea, N., et al. \| ApJ \| 807-20 \| 2015 \| 2015ApJ...807L..20B \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...807L..20B Hard X-Ray Excess from the Magnificent Seven Neutron Stars \|Dessert, Christopher, Foster, Joshua W., \| ApJ \| 904-42 \| 2020 \| 2020ApJ...904...42D \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904...42D Axion Emission Can Explain a New Hard X-Ray Excess from Nearby Isolated Neutron Stars \|Buschmann, Malte, Co, Raymond T., et al. \| PhRvL \| 126-21102 \| 2021 \| 2021PhRvL.126b1102B \| http://ui.adsabs.harvard.edu/#abs/2021PhRvL.126b1102B 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 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	2003-10-27T17:46:20Z/2003-10-28T06:14:58Z
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	2003-10-28T00:00:00Z
Keywords	"mos soft response"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Fred Jansen XMM-Newton PS, 2003, 'MOS soft response and Contamination Monitoring', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-bll92jp