A dataset provided by the European Space Agency

Name: NRCO MOS cooling proposal
Published: 2002-11-09T00:00:00Z

Proposal ID	015696
Title	NRCO MOS cooling proposal
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0156960101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0156960201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0156960301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0156960401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0156960501
DOI	https://doi.org/10.5270/esa-ivqkif1
Principal Investigator, PI	Dr Fred Jansen
Abstract	No abstract found for current proposal (This is a scientific proposal for an ESA mission. For specific information please contact ESDC Helpdesk - https://support.cosmos.esa.int/esdc)
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 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 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 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 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 New Optical/Ultraviolet Counterparts and the Spectral Energy Distributions of Nearby, Thermally Emitting, Isolated Neutron Stars \|Kaplan, D. L., Kamble, A., et al. \| ApJ \| 736-117 \| 2011 \| 2011ApJ...736..117K \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...736..117K A phase-dependent absorption line in the spectrum of the X-ray pulsar RX J0720.4-3125 \|Haberl, F., Zavlin, V. E., et al. \| A&A \| 419-1077 \| 2004 \| 2004A&A...419.1077H \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419.1077H ESO imaging survey: optical follow-up of 12 selected XMM-Newton fields \|Dietrich, J. P., Miralles, J.-M., et al. \| A&A \| 449-837 \| 2006 \| 2006A&A...449..837D \| http://ui.adsabs.harvard.edu/#abs/2006A&A...449..837D 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 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 The magnificent seven: magnetic fields and surface temperature distributions \|Haberl, Frank, \| Ap&SS \| 308-181 \| 2007 \| 2007Ap&SS.308..181H \| http://ui.adsabs.harvard.edu/#abs/2007Ap&SS.308..181H 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 Timing analysis of the isolated neutron star RX J0720.4-3125 revisited \|Cropper, Mark, Haberl, Frank, et al. \| MNRAS \| 351-1099 \| 2004 \| 2004MNRAS.351.1099C \| http://ui.adsabs.harvard.edu/#abs/2004MNRAS.351.1099C 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 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 serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P Nonthermal emission properties of the northwestern rim of supernova remnant RX J0852.0-4622 \|Kishishita, T., Hiraga, J., \| A&A \| 551-132 \| 2013 \| 2013A&A...551A.132K \| http://ui.adsabs.harvard.edu/#abs/2013A&A...551A.132K 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 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 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 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 The Magnificent Seven in the dusty prairie \|Posselt, B., Popov, S. B., et al. \| Ap&SS \| 308-171 \| 2007 \| 2007Ap&SS.308..171P \| http://ui.adsabs.harvard.edu/#abs/2007Ap&SS.308..171P The compactness of the isolated neutron star RX J0720.4-3125 \|Hambaryan, V., Suleimanov, V., et al. \| A&A \| 601-108 \| 2017 \| 2017A&A...601A.108H \| http://ui.adsabs.harvard.edu/#abs/2017A&A...601A.108H 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 Cyclotron lines in highly magnetized neutron stars \|Staubert, R., Trumper, J., et al. \| A&A \| 622-61 \| 2019 \| 2019A&A...622A..61S \| http://ui.adsabs.harvard.edu/#abs/2019A&A...622A..61S Universal detection of high-temperature emission in X-ray isolated neutron stars \|Yoneyama, Tomokage, Hayashida, Kiyoshi, et al. \| PASJ \| 71-17 \| 2019 \| 2019PASJ...71...17Y \| http://ui.adsabs.harvard.edu/#abs/2019PASJ...71...17Y 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 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 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	2002-11-06T01:34:21Z/2002-11-09T04:19:01Z
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	2002-11-09T00:00:00Z
Keywords	"nrco mos cooling"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Fred Jansen, 2002, 'NRCO MOS cooling proposal', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ivqkif1