A dataset provided by the European Space Agency

Name: Resolving Low energy lines from LMXRB
Published: 2002-07-27T00:00:00Z

Proposal ID	006114
Title	Resolving Low energy lines from LMXRB
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0061140101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0061140201
DOI	https://doi.org/10.5270/esa-27apolb
Principal Investigator, PI	Dr Lorella Angelini
Abstract	ASCA obsevations of the LMXRB X0918-54,X1543-62 and X0614+09 reveal strongemission lines in the 0.5-1 keV band.The emission is consistent with O and Fe L,but major uncertanties remain in establishing the line emission mechanism. Therecombination continuum,a signature of photoionization, is missing or at lowerlevel in all systems. A collisional plasma better reproduces the spectrum.Scattering and 3-body recombinations are other possible mechanism that can lowerthe recombination.We propose to observe X0918-54 and X1543-62 with the XMMgratings.These observations will differentiate line emission with anunprecedented resolving power. This capability will pin down the mechanismresponsible for the line emission, and define abundances to constrain the system
Publications	X-Ray Spectroscopy of the Low-Mass X-Ray Binaries 2S 0918-549 and 4U 1543-624: Evidence for Neon-rich Degenerate Donors \|Juett, Adrienne M., Chakrabarty, Deepto, \| ApJ \| 599-498 \| 2003 \| 2003ApJ...599..498J \| http://ui.adsabs.harvard.edu/#abs/2003ApJ...599..498J A systematic analysis of the broad iron Kalpha line in neutron-star LMXBs with XMM-Newton \|Ng, C., Diaz Trigo, M., et al. \| A&A \| 522-96 \| 2010 \| 2010A&A...522A..96N \| http://ui.adsabs.harvard.edu/#abs/2010A&A...522A..96N 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 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 Discovery of a broad O VIII Lyalpha line in the ultracompact X-ray binary 4U 1543-624 \|Madej, O. K., Jonker, P. G., \| MNRAS \| 412-11 \| 2011 \| 2011MNRAS.412L..11M \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.412L..11M 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 Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog \|Georgakakis, A. E., Chavushyan, V., et al. \| MNRAS \| 367-1017 \| 2006 \| 2006MNRAS.367.1017G \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367.1017G 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 source catalogue \|Watson, M. G., Pye, J. P., et al. \| AN \| 324-89 \| 2003 \| 2003AN....324...89W \| http://ui.adsabs.harvard.edu/#abs/2003AN....324...89W The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton \|De Luca, A., Molendi, S., \| A&A \| 419-837 \| 2004 \| 2004A&A...419..837D \| http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D 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 X-ray diagnostics of chemical composition of the accretion disc and donor star in UCXBs - II. XMM-Newton observations \|Koliopanos, Filippos, Gilfanov, Marat, et al. \| MNRAS \| 442-2817 \| 2014 \| 2014MNRAS.442.2817K \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.442.2817K Investigating the mass of the intermediate mass black hole candidate HLX-1 with the slimbh model \|Straub, Odele, Godet, Olivier, et al. \| A&A \| 569-116 \| 2014 \| 2014A&A...569A.116S \| http://ui.adsabs.harvard.edu/#abs/2014A&A...569A.116S 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 Interstellar Dust Properties from a Survey of X-Ray Halos \|Valencic, Lynne A., Smith, Randall K., \| ApJ \| 809-66 \| 2015 \| 2015ApJ...809...66V \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...809...66V Oxygen, neon, and iron X-ray absorption in the local interstellar medium \|Gatuzz, Efrain, Garcia, Javier A., et al. \| A&A \| 588-111 \| 2016 \| 2016A&A...588A.111G \| http://ui.adsabs.harvard.edu/#abs/2016A&A...588A.111G 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 On the detectability of CO molecules in the interstellar medium via X-ray spectroscopy \|Joachimi, Katerine, Gatuzz, Efrain, et al. \| MNRAS \| 461-352 \| 2016 \| 2016MNRAS.461..352J \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.461..352J 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 The Spectrum of the Universe \|Hill, Ryley, Masui, Kiyoshi W., \| ApSpe \| 72-663 \| 2018 \| 2018ApSpe..72..663H \| http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H 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 Disappearance of the Fe K \\u03b1 emission line in ultracompact X-ray binaries 4U 1543-624 and Swift J1756.9-2508 \|Koliopanos, Filippos, Vasilopoulos, Georgios, et al. \| MNRAS \| 500-5603 \| 2021 \| 2021MNRAS.500.5603K \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.5603K The chemical composition of the accretion disc and donor star in ultra-compact X-ray binaries: A comprehensive X-ray analysis \|Koliopanos, Filippos, P\\u00e9ault, Mathias, et al. \| MNRAS \| 501-548 \| 2021 \| 2021MNRAS.501..548K \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.501..548K 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	2001-02-04T13:17:58Z/2001-05-05T14:23:12Z
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	2002-07-27T00:00:00Z
Keywords	"recombination continuum", "collisional plasma", "lower level", "XMM", "major uncertanties", "asca obsevations", "lmxrb x0918", "emission lines", "low energy lines", "body recombinations", "kev band", "line emission mechanism", "line emission", "xmm gratings"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Lorella Angelini, 2002, 'Resolving Low energy lines from LMXRB', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-27apolb