A dataset provided by the European Space Agency

Name: XMM-Newton and MAGIC simultaneous observations of the gamma-ray binary LSI+61303
Published: 2008-11-14T00:00:00Z

Proposal ID	050598
Title	XMM-Newton and MAGIC simultaneous observations of the gamma-ray binary LSI+61303
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505980801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505980901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505981001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505981101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505981201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505981301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505981401
DOI	https://doi.org/10.5270/esa-y5696js
Principal Investigator, PI	Prof Josep Maria Paredes
Abstract	LS I +61 303 is a high mass X-ray binary that has been recently detected as avariable TeV source by MAGIC. We propose to conduct, for the first time,simultaneous X-ray and TeV observations, complemented with a radio monitoring,during several consecutive days centered around the orbital phase where themaximum TeV activity takes place. These observations will allow us to followinter-day spectral variability at X-ray and TeV energies. They will provide abetter sampled evolution of the X-ray flux and photon index around the phaseswhere X-ray outbursts are detected. They will also allow to verify the higherflux - harder spectrum correlation and the apparent non-existence of spectrallines. All this will be crucial to constrain physical properties of the emitter.
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 Correlated X-Ray and Very High Energy Emission in the Gamma-Ray Binary LS I +61 303 \|Anderhub, H., Antonelli, L. A., et al. \| ApJ \| 706-27 \| 2009 \| 2009ApJ...706L..27A \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...706L..27A On the origin of correlated X-ray/VHE emission from LS I +61 303 \|Zabalza, V., Paredes, J. M., \| A&A \| 527-9 \| 2011 \| 2011A&A...527A...9Z \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A...9Z 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 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 An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H 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 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 An XMM-Newton view of FeKalpha in high-mass X-ray binaries \|Gimenez-Garcia, A., Torrejon, J. M., et al. \| A&A \| 576-108 \| 2015 \| 2015A&A...576A.108G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...576A.108G 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 Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 Observational and theoretical study of the point sources of very high energy gamma-ray emission \|Babyk, Iurii, \| PhDT \| 0-5 \| 2017 \| 2017PhDT.........5B \| http://ui.adsabs.harvard.edu/#abs/2017PhDT.........5B Study of orbital and superorbital variability of LSI +61 303 with X-ray data \|Chernyakova, M., Babyk, Iu., et al. \| MNRAS \| 470-1718 \| 2017 \| 2017MNRAS.470.1718C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470.1718C 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 black hole candidate LS I +610303 \|Massi, M., Migliari, S., \| MNRAS \| 468-3689 \| 2017 \| 2017MNRAS.468.3689M \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468.3689M 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 Evidence for periodic accretion-ejection in LS I +61\\u00b0303 \|Massi, M., Chernyakova, M., et al. \| MNRAS \| 498-3592 \| 2020 \| 2020MNRAS.498.3592M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.498.3592M An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Modelling the correlated keV/TeV light curves of Be/gamma-ray binaries \|Chen, A. M., Takata, J., \| A&A \| 658-153 \| 2022 \| 2022A&A...658A.153C \| http://ui.adsabs.harvard.edu/#abs/2022A&A...658A.153C The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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 Discovering the Mass-Scaled Damping Timescale from Microquasars to Blazars \|Zhang, Haoyang, Yang, Shenbang, \| ApJ \| 967-L18 \| 2024 \| 2024ApJ...967L..18Z \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...967L..18Z 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	2007-09-04T01:48:30Z/2007-09-11T05:29:20Z
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	2008-11-14T00:00:00Z
Keywords	"spectral lines", "XMM", "constrain physical properties", "variable tev source", "orbital phase", "xray flux", "spectral variability", "tev energies", "XMM-Newton", "mass xray binary", "photon index", "xray outburst", "sampled evolution", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Josep Maria Paredes, 2008, 'XMM-Newton and MAGIC simultaneous observations of the gamma-ray binary LSI+61303', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-y5696js