A dataset provided by the European Space Agency

Name: Neutron Star Transient LMXBs; Catching Accreting Millisecond X-ray Pulsars
Published: 2017-03-18T23:00:00Z

Proposal ID	072255
Title	Neutron Star Transient LMXBs; Catching Accreting Millisecond X-ray Pulsars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722550301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722550401
DOI	https://doi.org/10.5270/esa-x1erhfl
Principal Investigator, PI	Prof Craig Heinke
Abstract	We propose two 32 ks ToO observations of newly identified, faint neutron starlow-mass X-ray binaries. The pn camera, in timing mode, can identify pulsationsfrom new accreting millisecond pulsars, measuring their spin and orbital period,along with studying any X-ray bursts. pn spectroscopy will study the continuumcomponents and broad lines, while RGS spectroscopy can search for narrowabsorption lines.
Publications	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 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	2013-03-28T18:44:09Z/2016-02-26T16:00:13Z
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	2017-03-18T23:00:00Z
Last Update	2025-01-27
Keywords	"broad lines", "xray bursts", "orbital period", "continuum components", "pn spectroscopy", "pn camera", "rgs spectroscopy", "accreting millisecond pulsars", "narrow absorption lines"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Craig Heinke, 2017, 'Neutron Star Transient LMXBs; Catching Accreting Millisecond X-ray Pulsars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-x1erhfl