A dataset provided by the European Space Agency

Name: Bright X-ray counterparts of galactic 3FGL sources
Published: 2018-06-19T22:00:00Z

Proposal ID	080293
Title	Bright X-ray counterparts of galactic 3FGL sources
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0802930101
DOI	https://doi.org/10.5270/esa-m15bwzq
Principal Investigator, PI	Mr Jeremy Hare
Abstract	We propose to follow-up the most interesting X-ray sources discovered during thesurvey of unidentified Fermi sources that we carried out with Swift. The surveytargeted a sub-sample of Fermi sources that we expect to be dominated by pulsarsalong with HMXBs, PWNe, and SNRs. In the proposed deeper XMM-Newton observationswe aim to constrain the spectrum of the 3 brightest sources, as well as searchfor variabilities, periodicities, and extended emission. Identifying the natureof these sources will allow us to better understand the population of galacticparticle accelerators, in particular, pulsars, PWNe, and HMXBs detected in bothgamma-rays and X-rays. We will also be able to search for much fainter X-raysources.
Publications	XMM-Newton and Chandra Observations of the Unidentified Fermi-LAT Source 3FGL J1016.5--6034: A Young Pulsar with a Nebula? \|Hare Jeremy Volkov Igor et al. \| ApJ \| 875-107 \| 2019 \| 2019ApJ...875..107H \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...875..107H 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 XMM-Newton and Chandra Observations of the Candidate Fermi-LAT Pulsar 4FGL J1015.5-6030 \|Hare Jeremy Kargaltsev Oleg et al. \| ApJ \| 951-80 \| 2023 \| 2023ApJ...951...80H \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...951...80H 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	2017-05-25T00:45:31Z/2017-05-25T05:45:31Z
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	2018-06-19T22:00:00Z
Last Update	2025-01-27
Keywords	"brightest sources", "fermi sources", "unidentified fermi sources", "sub sample", "supernova remnant", "XMM-Newton", "deeper xmm newton", "xray sources", "galactic particle accelerators", "fainter xray sources", "XMM", "survey targeted", "gamma rays", "galactic 3fgl sources", "bright xray counterparts"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Jeremy Hare, 2018, 'Bright X-ray counterparts of galactic 3FGL sources', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-m15bwzq