A dataset provided by the European Space Agency

Proposal ID	070120
Title	Hard X-ray study of the ultra-compact X-ray binary 4U 0614+091
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701200101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0701200201
DOI	https://doi.org/10.5270/esa-vfuxds2
Principal Investigator, PI	Dr Jerome Chenevez
Abstract	We propose a dedicated INTEGRAL monitoring program of the ultra-compact X-raybinary and micro-quasar 4U0614+091 to study its emission properties in hardX-rays. 4U0614+091 harbours the closest active X-ray burster, it exhibitsvariations on different time scales over the electromagnetic spectrum, such assynchrotron jet emission, X-ray flaring states, and thermonuclear X-ray bursts.Moreover, the high energy persistent emission is characterised by a particularlyhard (non thermal) X-ray tail. We want to survey the dynamical behaviour, betterdescribe its spectrum in hard X-rays, to follow the evolution of the long termpersistent emission variability, and to investigate the activity of shorter timescale processes. We request joint XMM and INTEGRAL observations.
Publications	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 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 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	EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-03-09T00:51:18Z/2013-09-09T05:05:34Z
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	2014-09-19T00:00:00Z
Keywords	"energy persistent emission", "hard xray", "emission properties", "XMM", "091 harbours", "time scales", "micro quasar 4u0614", "thermonuclear xray bursts", "thermal xray tail", "dedicated integral", "electromagnetic spectrum", "synchrotron jet emission", "xray flaring"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Jerome Chenevez, 2014, 'Hard X-ray study of the ultra-compact X-ray\n binary 4U 0614+091', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-vfuxds2