A dataset provided by the European Space Agency

Name: AEGIS_1862_24: Relic Jets from a Stellar Mass Galactic Object
Published: 2015-01-23T23:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	072338
Title	AEGIS_1862_24: Relic Jets from a Stellar Mass Galactic Object
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723380101
DOI	https://doi.org/10.5270/esa-7mm23ub
Principal Investigator, PI	Dr Sean Farrell
Abstract	We request a single XMM-Newton observation of a recently discovered Galacticsystem with possible large scale relic jets. The optical spectrum of this sourceis consistent with accretion disc emission from a binary system. Two extendednon-thermal optical sources are symmetrically located 3.4 either side of thecentral object, consistent with relic jet lobes. Faint X-ray emission wasdetected from this source with Swift, consistent with a quiescent low mass X-raybinary or an intermediate polar. Relic jets from X-ray binaries are extremelyrare, and such large scale jets from an intermediate polar have never been seenbefore. Through this observation we aim to determine the nature of this objectby constraining the X-ray spectral and timing properties of the central source.
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 SMSS J130522.47-293113.0: a high-latitude stellar X-ray source with pc-scale outflow relics? \|Da Costa G. S. Soria R. et al. \| MNRAS \| 477-766 \| 2018 \| 2018MNRAS.477..766D \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.477..766D 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 Dynamical state of galaxy clusters evaluated from X-ray images \|Yuan Z. S. Han J. L. \| MNRAS \| 513-3013 \| 2022 \| 2022MNRAS.513.3013Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.3013Y The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2014-01-12T04:21:29Z/2014-01-13T01:59:49Z
Version	21.51_20241115_1113
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	2015-01-23T23:00:00Z
Last Update	2026-06-19
Keywords	"xray binary", "intermediate polar", "galactic system", "XMM-Newton", "central source", "faint xray emission", "single xmm newton", "relic jets", "binary system", "accretion disc emission", "scale relic jets", "central object", "nonthermal optical sources", "relic jet lobes", "optical spectrum", "scale jets", "XMM", "symmetrically located", "xray spectral"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Sean Farrell, 2015, 'AEGIS_1862_24: Relic Jets from a Stellar Mass Galactic Object', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-7mm23ub
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.