A dataset provided by the European Space Agency

Name: The multiwavelength light curve of X1822-371 SSC_47
Published: 2002-05-26T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	011123
Title	The multiwavelength light curve of X1822-371 SSC_47
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111230101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111230201
DOI	https://doi.org/10.5270/esa-nkt9a3n
Principal Investigator, PI	Dr Michael Watson
Abstract	GT-The X-ray and ultraviolet light curves of X1822-371 will be measured overthree 5.57 hour binary cycles in order to study the relationship of theaccretion disk corona to the disk, and to measure the disk geometry. The X-rayspectrum of the source will be measured as a function of the binary phase,making use of the phase dependent obscuration of the accretion disk corona toseparate different spatial components of the emission.
Publications	New ephemeris of the ADC source 2A 1822-371: a stable orbital-period derivative over 30 years \|Burderi L. Di Salvo T. et al. \| A&A \| 515-44 \| 2010 \| 2010A&A...515A..44B \| http://ui.adsabs.harvard.edu/#abs/2010A&A...515A..44B 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 Phase-resolved optical and X-ray spectroscopy of low-mass X-ray binary X1822-371 \|Somero A. Hakala P. et al. \| A&A \| 539-111 \| 2012 \| 2012A&A...539A.111S \| http://ui.adsabs.harvard.edu/#abs/2012A&A...539A.111S 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 New measurement of orbital and spin period evolution of the accretion disc corona source 4U 1822-37 \|Jain Chetana Paul Biswajit \| MNRAS \| 409-755 \| 2010 \| 2010MNRAS.409..755J \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.409..755J 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 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 X-ray spectroscopy of the ADC source X1822-371 with Chandra and XMM-Newton \|Iaria R. Di Salvo T. et al. \| A&A \| 549-33 \| 2013 \| 2013A&A...549A..33I \| http://ui.adsabs.harvard.edu/#abs/2013A&A...549A..33I 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 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 A possible cyclotron resonance scattering feature near 0.7 keV in X1822-371 \|Iaria R. Di Salvo T. et al. \| A&A \| 577-63 \| 2015 \| 2015A&A...577A..63I \| http://ui.adsabs.harvard.edu/#abs/2015A&A...577A..63I Sunyaev-Zeldovich 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 Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton RXTE and INTEGRAL observations \|Duro Refiz Dauser Thomas et al. \| A&A \| 589-14 \| 2016 \| 2016A&A...589A..14D \| http://ui.adsabs.harvard.edu/#abs/2016A&A...589A..14D 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 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 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 Confirmation of the presence of a CRSF in the NICER spectrum of X 1822-371 \|Iaria R. Di Salvo T. et al. \| A&A \| 683-A79 \| 2024 \| 2024A&A...683A..79I \| http://ui.adsabs.harvard.edu/#abs/2024A&A...683A..79I 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 Probing the inner Galactic halo with blue horizontal-branch stars. Gaia DR3-based catalogue with atmospheric and stellar parameters \|Culpan R. Dorsch M. et al. \| A&A \| 685-A134 \| 2024 \| 2024A&A...685A.134C \| http://ui.adsabs.harvard.edu/#abs/2024A&A...685A.134C New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2001-03-07T09:56:09Z/2001-03-08T03:35:17Z
Version	21.51_20241115_1113
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	2002-05-26T00:00:00Z
Last Update	2026-07-09
Keywords	"spatial components", "multiwavelength light curve", "binary phase", "x1822 371 ssc_47", "binary cycles", "x1822 371", "phase dependent obscuration", "xray spectrum", "ultraviolet light curves", "accretion disk corona", "disk geometry", "X1822-371"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Michael Watson, 2002, 'The multiwavelength light curve of X1822-371 SSC_47', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-nkt9a3n
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.