A dataset provided by the European Space Agency

Name: High Resolution Spectroscopy of 4U0614+09
Published: 2002-07-23T00:00:00Z

Proposal ID	011104
Title	High Resolution Spectroscopy of 4U0614+09
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111040101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0111040201
DOI	https://doi.org/10.5270/esa-zvx1tt9
Principal Investigator, PI	Dr Albert Brinkman
Abstract	GT- We will obtain a very high signal-to-noise, high resolution spectrumof the bright Low Mass X-ray Binary 4U0614+09. CCD spectroscopy hasindicated that surprisingly large EW discrete emission is present inthe spectrum below 1 keV. With the RGS spectrum, we will resolve thisemission, infer its origin, and the physical conditions in the source.The source is bright enough that one RGS will be run in high timeresolution mode, to study a possible dependence of the discreteemission on the continuum flux.
Publications	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 relativistically broadened OVIII Lyalpha line in the ultracompact X-ray binary 4U 0614+091 \|Madej O. K. Jonker P. G. et al. \| MNRAS \| 407-11 \| 2010 \| 2010MNRAS.407L..11M \| http://ui.adsabs.harvard.edu/#abs/2010MNRAS.407L..11M The interstellar oxygen-K absorption edge as observed by XMM-Newton. Separation of instrumental and interstellar components \|de Vries C. P. den Herder J. W. et al. \| A&A \| 404-959 \| 2003 \| 2003A&A...404..959D \| http://ui.adsabs.harvard.edu/#abs/2003A&A...404..959D 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 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 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 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 X-ray reflection in oxygen-rich accretion discs of ultracompact X-ray binaries \|Madej O. K. Garcia J. et al. \| MNRAS \| 442-1157 \| 2014 \| 2014MNRAS.442.1157M \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.442.1157M 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 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 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 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 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 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 NuSTAR Observations of the Accreting Atolls GX 3+1 4U 1702-429 4U 0614+091 and 4U 1746-371 \|Ludlam R. M. Miller J. M. et al. \| ApJ \| 873-99 \| 2019 \| 2019ApJ...873...99L \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...873...99L 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 chemical composition of the accretion disc and donor star in ultra-compact X-ray binaries: A comprehensive X-ray analysis \|Koliopanos Filippos Pu00e9ault 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 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	2001-03-13T09:35:10Z/2001-03-13T17:31:02Z
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	2002-07-23T00:00:00Z
Last Update	2025-01-27
Keywords	"resolution spectroscopy", "ew discrete emission", "ccd spectroscopy", "physical conditions", "discrete emission", "continuum flux", "time resolution mode", "rgs spectrum", "resolution spectrum"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Albert Brinkman, 2002, 'High Resolution Spectroscopy of 4U0614+09', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-zvx1tt9