A dataset provided by the European Space Agency

Name: Characterization of the most highly-ionized absorbers in dipping LMXBs
Published: 2009-01-01T00:00:00Z

Proposal ID	040551
Title	Characterization of the most highly-ionized absorbers in dipping LMXBs
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405510201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405510301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405510401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405510501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405510601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405510701
DOI	https://doi.org/10.5270/esa-mpw9veg
Principal Investigator, PI	Dr Maria Diaz Trigo
Abstract	We propose three 60 ksec and one 140 ks XMM-Newton observations of the dippingLow-Mass X-ray Binaries (LMXBs) XB 1254-690 and 4U 1746-371. We will obtain upto ~12 ks of dip data per 4U 1254-690 observation which will be sufficient toreliably measure the dip properties and the changes in the absorber, compared tothe persistent emission. The 140 ks of the 4U 1746-12 observation, added to aprevious 50 ks XMM-Newton observation on this source, will be enough to detectwith high significance the Fe XXVI absorption feature seen in the previousobservation at low confidence in the persistent emission and Fe XXV and/or FeXXVI absorption features in the dipping emission. The significant detection ofthese lines will allow the absorber properties to be unambigously characterized.
Publications	Variations in the dip properties of the low-mass X-ray binary XB 1254-690 observed with XMM-Newton and INTEGRAL \|Diaz Trigo M. Parmar A. N. et al. \| A&A \| 493-145 \| 2009 \| 2009A&A...493..145D \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..145D 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 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 Interstellar medium composition through X-ray spectroscopy of low-mass X-ray binaries \|Pinto C. Kaastra J. S. et al. \| A&A \| 551-25 \| 2013 \| 2013A&A...551A..25P \| http://ui.adsabs.harvard.edu/#abs/2013A&A...551A..25P 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 XMM-Newton observations reveal the disappearance of the wind in 4U 1630-47 \|Diaz Trigo M. Migliari S. et al. \| A&A \| 571-76 \| 2014 \| 2014A&A...571A..76D \| http://ui.adsabs.harvard.edu/#abs/2014A&A...571A..76D 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 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 The composition of the interstellar medium in the Galaxy as seen through X-rays \|Pinto Ciro \| PhDT \| 0-3 \| 2013 \| 2013PhDT.........3P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.........3P Updating the orbital ephemeris of the dipping source XB 1254-690 and the distance to the source \|Gambino Angelo F. Iaria Rosario et al. \| RAA \| 17-108 \| 2017 \| 2017RAA....17..108G \| http://ui.adsabs.harvard.edu/#abs/2017RAA....17..108G 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 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 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 Properties of Milky Way globular clusters associated with X-ray sources \|Botev Svetoslav Nedialkov Petko \| BlgAJ \| 40-59 \| 2024 \| 2024BlgAJ..40...59B \| http://ui.adsabs.harvard.edu/#abs/2024BlgAJ..40...59B 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	2006-09-12T15:00:39Z/2007-03-09T20:45:47Z
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	2009-01-01T00:00:00Z
Last Update	2025-01-27
Keywords	"persistent emission", "dipping emission", "fe xxvi absorption", "unambigously characterized", "4u 1746", "xmm newton", "dip properties", "fe xxv", "XMM-Newton", "dip data", "4u 1254 690", "4u 1746 371", "XMM", "low confidence", "140 xmm newton", "dipping lmxbs", "ionized absorbers", "absorber properties"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Maria Diaz Trigo, 2009, 'Characterization of the most highly-ionized absorbers in dipping LMXBs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mpw9veg