A dataset provided by the European Space Agency

Name: Long-term evolution of the fastest accreting millisecond pulsar IGR J00291+5934
Published: 2016-08-05T22:00:00Z

Proposal ID	074484
Title	Long-term evolution of the fastest accreting millisecond pulsar IGR J00291+5934
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744840201
DOI	https://doi.org/10.5270/esa-028xlgn
Principal Investigator, PI	Dr Alessandro Papitto
Abstract	We propose a 70 ks XMM observation of the fastest accreting millisecond pulsardiscovered so far, IGR J00291+5934, during its next outburst. A measure of itsspin and orbital parameters will put firm constraints on its long-term evolutionand on the mechanisms (magneto-dipole emission, gravitational radiation)proposed to explain it. The lack of neutron stars observed to spin atfrequencies close the centrifugal break-up (virgul1.5 kHz) will be tackled on anobservational basis. The observation will also give accurate pulsar ephemeris,to allow a search for the gamma-ray counterpart expected to turn on as thesource switches to a rotation-powered pulsar state during X-ray quiescence. Thisis a re-submission of a proposal approved for the AO11 and 12, and which was not triggered.
Publications	Discovery of a soft X-ray 8 mHz QPO from the accreting millisecond pulsar IGR J00291+5934 \|Ferrigno, C., Bozzo, E., et al. \| MNRAS \| 466-3450 \| 2017 \| 2017MNRAS.466.3450F \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.466.3450F The Slow Orbital Evolution of the Accreting Millisecond Pulsar IGR J0029+5934 \|Patruno, Alessandro, \| ApJ \| 839-51 \| 2017 \| 2017ApJ...839...51P \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...839...51P Quasi-periodic Pulse Amplitude Modulation in the Accreting Millisecond Pulsar IGR J00291+5934 \|Bult, Peter, van Doesburgh, Marieke, \| ApJ \| 845-124 \| 2017 \| 2017ApJ...845..124B \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...845..124B Rapid X-ray variability properties during the unusual very hard state in neutron-star low-mass X-ray binaries \|Wijnands, R., Parikh, A. S., et al. \| MNRAS \| 472-559 \| 2017 \| 2017MNRAS.472..559W \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.472..559W Quasi-simultaneous INTEGRAL, SWIFT, and NuSTAR Observations of the New X-Ray Clocked Burster 1RXS J180408.9-342058 \|Fiocchi, M., Bazzano, A., et al. \| ApJ \| 887-30 \| 2019 \| 2019ApJ...887...30F \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...887...30F 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 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	2015-07-28T11:48:19Z/2015-07-29T11:51:02Z
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	2016-08-05T22:00:00Z
Keywords	"orbital parameters", "neutron stars", "firm constraints", "XMM", "centrifugal break", "gamma ray counterpart", "gravitational radiation", "source switches", "frequencies close", "pulsar ephemeris", "re submission", "igr j00291", "term evolution", "rotation powered pulsar", "xray quiescence"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Alessandro Papitto, 2016, 'Long-term evolution of the fastest accreting millisecond pulsar IGR J00291+5934', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-028xlgn