A dataset provided by the European Space Agency

Name: XMM SEARCH FOR PROTON CYCLOTRON FEATURES IN IN THE AXP 4U0142+614
Published: 2005-08-29T00:00:00Z

Proposal ID	020667
Title	XMM SEARCH FOR PROTON CYCLOTRON FEATURES IN IN THE AXP 4U0142+614
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0206670101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0206670201
DOI	https://doi.org/10.5270/esa-pagwxax
Principal Investigator, PI	Dr NANDA REA
Abstract	The magnetar.. model, proposed to account for the nature of the X-ray emissionfrom AXPs, assume that these sources are powered by magnetic field decay of amagnetic field strength of >10^14 Gauss. If the magnetar scenario is correct,proton cyclotron features (PCFs) are expected to lie in the X-ray band. Wepropose an XMM observation of the 4U0142+614, the brightest source of this classof pulsars. The present request is first aimed at searching for an absorptionfeature due to proton cyclotron scattering, that would allow us to finally inferits magnetic field strenght. Secondly, we will study the link between timing andspectral properties. Finally, we will check for the presence of a broad spectralfeature we marginally detected during a ASCA 2001 observation.
Publications	Extinction Columns and Intrinsic X-Ray Spectra of the Anomalous X-Ray Pulsars \|Durant, Martin, van Kerkwijk, Marten H., \| ApJ \| 650-1082 \| 2006 \| 2006ApJ...650.1082D \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...650.1082D Detailed high-energy characteristics of AXP 4U 0142+61. Multi-year observations with INTEGRAL, RXTE, XMM-Newton, and ASCA \|den Hartog, P. R., Kuiper, L., et al. \| A&A \| 489-245 \| 2008 \| 2008A&A...489..245D \| http://ui.adsabs.harvard.edu/#abs/2008A&A...489..245D Long-term X-ray Changes in the Emission from the Anomalous X-ray Pulsar 4U 0142+61 \|Gonzalez, M. E., Dib, R., et al. \| ApJ \| 716-1345 \| 2010 \| 2010ApJ...716.1345G \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...716.1345G 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 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 Very deep X-ray observations of the anomalous X-ray pulsar 4U0142+614 \|Rea, N., Nichelli, E., et al. \| MNRAS \| 381-293 \| 2007 \| 2007MNRAS.381..293R \| http://ui.adsabs.harvard.edu/#abs/2007MNRAS.381..293R X-ray spectra from magnetar candidates - III. Fitting SGR/AXP soft X-ray emission with non-relativistic Monte Carlo models \|Zane, S., Rea, N., et al. \| MNRAS \| 398-1403 \| 2009 \| 2009MNRAS.398.1403Z \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.398.1403Z Multiwavelength Variability of the Magnetar 4U 0142+61 \|Durant, Martin, van Kerkwijk, Marten H., \| ApJ \| 652-576 \| 2006 \| 2006ApJ...652..576D \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...652..576D Physical Properties of the AXP 4U 0142+61 from X-Ray Spectral Analysis \|Guver, Tolga, Ozel, Feryal, \| ApJ \| 675-1499 \| 2008 \| 2008ApJ...675.1499G \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...675.1499G 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 Resonant Cyclotron Scattering in Magnetars. Emission \|Rea, N., Zane, S., et al. \| ApJ \| 686-1245 \| 2008 \| 2008ApJ...686.1245R \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...686.1245R 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 Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey \|Pineau, F.-X., Motch, C., et al. \| A&A \| 527-126 \| 2011 \| 2011A&A...527A.126P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.126P Exploring X-ray and radio emission of type 1 AGN up to z virgul 2.3 \|Ballo, L., Heras, F. J. H., et al. \| A&A \| 545-66 \| 2012 \| 2012A&A...545A..66B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution models \|Vigano, D., Rea, N., et al. \| MNRAS \| 434-123 \| 2013 \| 2013MNRAS.434..123V \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.434..123V 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 X-Ray Perspective of the Twisted Magnetospheres of Magnetars \|Weng, Shan-Shan, Gogus, Ersin, et al. \| ApJ \| 805-81 \| 2015 \| 2015ApJ...805...81W \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...805...81W Phase-resolved X-Ray Spectra of Magnetars and the Coronal Outflow Model \|Hascoet, Romain, Beloborodov, Andrei M., \| ApJ \| 786-1 \| 2014 \| 2014ApJ...786L...1H \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786L...1H 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 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 Magnetic fields in neutron stars \|Vigano, Daniele, \| PhDT \| 0-7 \| 2013 \| 2013PhDT.........7V \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.........7V Intrinsic spectra of the AXPs \|Durant, Martin, \| Ap&SS \| 308-641 \| 2007 \| 2007Ap&SS.308..641D \| http://ui.adsabs.harvard.edu/#abs/2007Ap&SS.308..641D Systematic study of magnetar outbursts \|Coti Zelati, Francesco, Rea, Nanda, et al. \| MNRAS \| 474-961 \| 2018 \| 2018MNRAS.474..961C \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.474..961C 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 The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars \|Papitto, A., Falanga, M., et al. \| NewAR \| 91-101544 \| 2020 \| 2020NewAR..9101544P \| http://ui.adsabs.harvard.edu/#abs/2020NewAR..9101544P 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 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	2004-03-01T09:16:55Z/2004-07-25T10:16:20Z
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	2005-08-29T00:00:00Z
Keywords	"magnetic field strength", "xray band", "magnetar scenario", "magnetic field strenght", "magnetic field decay", "XMM", "proton cyclotron", "asca 2001", "axp 4u0142", "xmm search", "spectral properties", "xray emission", "broad spectral", "proton cyclotron scattering", "brightest source"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr NANDA REA, 2005, 'XMM SEARCH FOR PROTON CYCLOTRON FEATURES IN IN THE AXP 4U0142+614', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-pagwxax