A dataset provided by the European Space Agency

Name: XMM-NEWTON OBSERVATIONS OF JUPITER AND ITS NEIGHBOURHOOD
Published: 2008-05-02T00:00:00Z

Proposal ID	020008
Title	XMM-NEWTON OBSERVATIONS OF JUPITER AND ITS NEIGHBOURHOOD
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080231 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080232 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080233 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080234 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080701 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080731 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080732 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080733 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080734 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200080901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0200081001
DOI	https://doi.org/10.5270/esa-f2ax0iw
Principal Investigator, PI	Dr GRAZIELLA BRANDUARDI-RAYMONT
Abstract	Jupiter and its neighbourhood are an exceptionally interesting source of X-rayswithin the solar system. We propose to observe the planet and its Galilean moonsover two XMM-Newton orbits. A good signal-to-noise RGS spectrum of Jupiter.sauroral .hot spots. will resolve the question of their origin: energetic ionprecipitation from entirely inside the magnetosphere, or acceleration ofcaptured solar wind ions in the outer magnetosphere. With EPIC we will studyoscillations observed by Chandra in the hot spot emissions, and the asymmetriesin Jupiter.s low-latitude X-ray emission first observed with ROSAT; we willstudy how Io.s and its Plasma Torus X-ray emissions vary with Io.s orbital phaseabout Jupiter, and we will obtain the first secure X-ray detections of all four Galilean satellites.
Publications	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 Comparative analysis and variability of the Jovian X-ray spectra detected by the Chandra and XMM-Newton observatories \|Hui, Yawei, Schultz, David R., et al. \| JGRA \| 115-7102 \| 2010 \| 2010JGRA..115.7102H \| http://ui.adsabs.harvard.edu/#abs/2010JGRA..115.7102H Solar control on Jupiter.s equatorial X-ray emissions: 26-29 November 2003 XMM-Newton observation \|Bhardwaj, Anil, Branduardi-Raymont, G., et al. \| GeoRL \| 32-308 \| 2005 \| 2005GeoRL..32.3S08B \| http://ui.adsabs.harvard.edu/#abs/2005GeoRL..32.3S08B A study of Jupiter.s aurorae with XMM-Newton \|Branduardi-Raymont, G., Bhardwaj, A., et al. \| A&A \| 463-761 \| 2007 \| 2007A&A...463..761B \| http://ui.adsabs.harvard.edu/#abs/2007A&A...463..761B Latest results on Jovian disk X-rays from XMM-Newton \|Branduardi-Raymont, G., Bhardwaj, A., et al. \| P&SS \| 55-1126 \| 2007 \| 2007P&SS...55.1126B \| http://ui.adsabs.harvard.edu/#abs/2007P&SS...55.1126B 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 The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C 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 X-rays from solar system objects \|Bhardwaj, Anil, Elsner, Ronald F., et al. \| P&SS \| 55-1135 \| 2007 \| 2007P&SS...55.1135B \| http://ui.adsabs.harvard.edu/#abs/2007P&SS...55.1135B Ensemble X-ray variability of active galactic nuclei from serendipitous source catalogues \|Vagnetti, F., Turriziani, S., \| A&A \| 536-84 \| 2011 \| 2011A&A...536A..84V \| http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..84V The 2XMMi/SDSS Galaxy Cluster Survey. III. Clusters associated with spectroscopically targeted luminous red galaxies in SDSS-DR10 \|Takey, A., Schwope, A., \| A&A \| 564-54 \| 2014 \| 2014A&A...564A..54T \| http://ui.adsabs.harvard.edu/#abs/2014A&A...564A..54T 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 Low- to middle-latitude X-ray emission from Jupiter \|Bhardwaj, Anil, Elsner, Ronald F., et al. \| JGRA \| 111-11225 \| 2006 \| 2006JGRA..11111225B \| http://ui.adsabs.harvard.edu/#abs/2006JGRA..11111225B 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 XMM-Newton Observations of X-Ray Emission from Jupiter \|Branduardi-Raymont, G., Bhardwaj, A., et al. \| aogs \| 3-203 \| 2006 \| 2006aogs....3..203B \| http://ui.adsabs.harvard.edu/#abs/2006aogs....3..203B SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 \|Pons, E., Watson, M. G., \| A&A \| 594-72 \| 2016 \| 2016A&A...594A..72P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..72P 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 Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals \|Sibeck, David G., Allen, R., et al. \| SSRv \| 214-79 \| 2018 \| 2018SSRv..214...79S \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S 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 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 X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C 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 Jupiter.s equatorial X-ray emissions over two solar cycles \|Wibisono, A. D., Branduardi-Raymont, G., et al. \| MNRAS \| 521-5596 \| 2023 \| 2023MNRAS.521.5596W \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.521.5596W 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, RGS1, RGS2
Temporal Coverage	2003-11-25T21:07:53Z/2003-11-29T12:17:22Z
Version	PPS_NOT_AVAILABLE
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	2008-05-02T00:00:00Z
Keywords	"secure xray detections", "hot spots", "XMM", "energetic ion precipitation", "solar system", "orbital phase", "galilean moons", "xmm newton orbits", "galilean satellites", "noise rgs spectrum", "XMM-Newton", "outer magnetosphere", "EPIC", "hot spot emissions", "ROSAT", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr GRAZIELLA BRANDUARDI-RAYMONT, 2008, 'XMM-NEWTON OBSERVATIONS OF JUPITER AND ITS NEIGHBOURHOOD', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-f2ax0iw