A dataset provided by the European Space Agency

Name: Monitoring the hydrogenic column density in obscured HMXB
Published: 2009-10-28T00:00:00Z

Proposal ID	055614
Title	Monitoring the hydrogenic column density in obscured HMXB
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556140101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556140201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556140301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556140401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556140501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556140601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556140701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556140801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0556141001
DOI	https://doi.org/10.5270/esa-uupqyp7
Principal Investigator, PI	Dr Juan Antonio Zurita Heras
Abstract	We request to monitor 4 obscured HMXB composed by a neutron star and asupergiant OB companion (IGR J16320-4751, IGR J16393-4643, IGR J16418-4532, IGRJ18027-2016 in order of preference) in order to study their spectral evolutionalong their orbital period, particularly the hydrogenic column density. We planto observe IGR J16320-4751 8 times 5 ks and IGR J16393-4643, IGR J16418-4532 andIGR J18027-2016 5 times 7 ks for a total of 145 ks. Because of the stronginteraction between the supergiant wind and the X-ray radiation of the accretedmaterial, these sources are ideal laboratories to study the relation between thecolumn density and the orbital period and derive the properties of the stellarwind.
Publications	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 Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C 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 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 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 An XMM-Newton view of FeKalpha in high-mass X-ray binaries \|Gimenez-Garcia A. Torrejon J. M. et al. \| A&A \| 576-108 \| 2015 \| 2015A&A...576A.108G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...576A.108G 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 HESS J1632-478: an energetic relic \|Balbo M. Saouter P. et al. \| A&A \| 520-111 \| 2010 \| 2010A&A...520A.111B \| http://ui.adsabs.harvard.edu/#abs/2010A&A...520A.111B Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants \|Prinz Tobias \| PhDT \| 0-305 \| 2013 \| 2013PhDT.......305P \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P Supergiant fast X-ray transients versus classical supergiant high mass X-ray binaries: Does the difference lie in the companion wind? \|Pradhan P. Bozzo E. \| A&A \| 610-50 \| 2018 \| 2018A&A...610A..50P \| http://ui.adsabs.harvard.edu/#abs/2018A&A...610A..50P Analisis temporal y espectral en rayos X de la fuente IGR J16320-4751 \|Fogantini F. Garcia F. et al. \| BAAA \| 60-98 \| 2018 \| 2018BAAA...60...98F \| http://ui.adsabs.harvard.edu/#abs/2018BAAA...60...98F Spectral evolution of the supergiant HMXB IGR J16320-4751 along its orbit using XMM-Newton \|Garcia Federico Fogantini Federico A. et al. \| A&A \| 618-61 \| 2018 \| 2018A&A...618A..61G \| http://ui.adsabs.harvard.edu/#abs/2018A&A...618A..61G 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 Peculiar temporal and spectral features in highly obscured HMXB pulsar IGR J16320-4751 using XMM-Newton \|Varun Iyer Nirmal \| NewA \| 98-101942 \| 2023 \| 2023NewA...9801942V \| http://ui.adsabs.harvard.edu/#abs/2023NewA...9801942V NuSTAR investigation of X-ray variability and hard X-ray spectral properties in IGR J16320-4751 and IGR J16479-4514 \|Varun Raman Gayathri \| MNRAS \| 523-5024 \| 2023 \| 2023MNRAS.523.5024V \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.523.5024V 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	2008-08-14T22:18:21Z/2008-09-17T03:39:30Z
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	2009-10-28T00:00:00Z
Last Update	2025-01-27
Keywords	"spectral evolution", "xray radiation", "obscured hmxb", "igr j18027 2016", "igr j16393 4643", "accreted material", "hydrogenic column density", "obscured hmxb composed", "orbital period", "column density", "igr j16418 4532", "ideal laboratories", "stellar wind", "neutron star", "supergiant wind", "igr j16320 4751"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Juan Antonio Zurita Heras, 2009, 'Monitoring the hydrogenic column density in obscured HMXB', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-uupqyp7