A dataset provided by the European Space Agency

Name: Probing the nature of the circumstellar environment around periastron in SFXTs
Published: 2013-10-09T00:00:00Z

Proposal ID	067981
Title	Probing the nature of the circumstellar environment around periastron in SFXTs
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0679810101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0679810201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0679810301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0679810401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0679810501
DOI	https://doi.org/10.5270/esa-ix1ec4e
Principal Investigator, PI	Dr Sebastian Drave
Abstract	To achieve the goals outlined in this proposal we request ~1.7 Ms of INTEGRALobservations complemented with 140 ks of simultaneous XMM-Newton observatons.
Publications	INTEGRAL and XMM-Newton observations of IGR J16418-4532: evidence of accretion regime transitions in a supergiant fast X-ray transient \|Drave S. P. Bird A. J. et al. \| MNRAS \| 433-528 \| 2013 \| 2013MNRAS.433..528D \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.433..528D New insights on accretion in supergiant fast X-ray transients from XMM-Newton and INTEGRAL observations of IGR J17544-2619 \|Drave S. P. Bird A. J. et al. \| MNRAS \| 439-2175 \| 2014 \| 2014MNRAS.439.2175D \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.439.2175D 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 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 accretion environment of supergiant fast X-ray transients probed with XMM-Newton \|Bozzo E. Bernardini F. et al. \| A&A \| 608-128 \| 2017 \| 2017A&A...608A.128B \| http://ui.adsabs.harvard.edu/#abs/2017A&A...608A.128B 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 X-ray chimneys in the Galactic Centre \|Chernyakova Masha \| Natur \| 567-318 \| 2019 \| 2019Natur.567..318C \| http://ui.adsabs.harvard.edu/#abs/2019Natur.567..318C An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre \|Ponti G. Hofmann F. et al. \| Natur \| 567-347 \| 2019 \| 2019Natur.567..347P \| http://ui.adsabs.harvard.edu/#abs/2019Natur.567..347P X-Ray Reprocessing: Through the Eclipse Spectra of High-mass X-Ray Binaries with XMM-Newton \|Aftab Nafisa Paul Biswajit \| ApJS \| 243-29 \| 2019 \| 2019ApJS..243...29A \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..243...29A Dust-scattering Halo and Giant Hard X-Ray Flare from the Supergiant Fast X-Ray Transient IGR J16479-4514 Investigated with XMM-Newton and INTEGRAL \|Sguera V. Tiengo A. et al. \| ApJ \| 900-22 \| 2020 \| 2020ApJ...900...22S \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...900...22S The Galactic center chimneys: the base of the multiphase outflow of the Milky Way \|Ponti G. Morris M. R. et al. \| A&A \| 646-66 \| 2021 \| 2021A&A...646A..66P \| http://ui.adsabs.harvard.edu/#abs/2021A&A...646A..66P 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 Tracing the Milky Ways Vestigial Nuclear Jet \|Cecil Gerald Wagner Alexander Y. et al. \| ApJ \| 922-254 \| 2021 \| 2021ApJ...922..254C \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...922..254C The episodic and multiscale Galactic Centre \|Bryant Aaron Krabbe Alfred \| NewAR \| 93-101630 \| 2021 \| 2021NewAR..9301630B \| http://ui.adsabs.harvard.edu/#abs/2021NewAR..9301630B X-ray astronomy comes of age \|Wilkes Belinda J. Tucker Wallace et al. \| Natur \| 606-261 \| 2022 \| 2022Natur.606..261W \| http://ui.adsabs.harvard.edu/#abs/2022Natur.606..261W 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 Scientific objectives of the Hot Universe Baryon Surveyor (HUBS) mission \|Bregman Joel Cen Renyue et al. \| SCPMA \| 66-299513 \| 2023 \| 2023SCPMA..6699513B \| http://ui.adsabs.harvard.edu/#abs/2023SCPMA..6699513B The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way \|Sarkar Kartick C. \| A&ARv \| 32-1 \| 2024 \| 2024A&ARv..32....1S \| http://ui.adsabs.harvard.edu/#abs/2024A&ARv..32....1S Energy dependence of quasi-periodic oscillations in accreting X-ray pulsars \|Manikantan Hemanth Paul Biswajit et al. \| MNRAS \| 531-530 \| 2024 \| 2024MNRAS.531..530M \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.531..530M 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	2012-08-21T11:30:20Z/2012-09-16T21:46:15Z
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	2013-10-09T00:00:00Z
Last Update	2025-01-27
Keywords	"xmm newton", "XMM-Newton", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Sebastian Drave, 2013, 'Probing the nature of the circumstellar environment around periastron in SFXTs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ix1ec4e