A dataset provided by the European Space Agency

Name: Is XGPS-25 an extreme ADC source ?
Published: 2014-03-26T00:00:00Z

Proposal ID	069492
Title	Is XGPS-25 an extreme ADC source ?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694920101
DOI	https://doi.org/10.5270/esa-w9vsarf
Principal Investigator, PI	Dr Christian Motch
Abstract	Our optical identification campaign of hard X-ray sources in the XMM-NewtonGalactic Plane Survey (XGPS) has revealed several exceptional objects. Amongthese is XGPS-25 which has all the features expected from a low-mass X-raybinary whose X-ray emission is strongly shielded by the accretion disc and ifconfirmed, would be the first very high inclination accretion disc corona knownto date. The present proposal aims at obtaining a high quality X-ray spectrumand time series which will help us to understand the nature of this object.
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	2013-03-15T05:58:08Z/2013-03-15T12:03:26Z
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	2014-03-26T00:00:00Z
Last Update	2025-01-27
Keywords	"adc source ?.", "XMM-Newton", "xray emission", "quality xray spectrum", "XMM", "time series", "optical identification campaign", "hard xray sources", "accretion disc"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Christian Motch, 2014, 'Is XGPS-25 an extreme ADC source ?', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-w9vsarf