A dataset provided by the European Space Agency

Name: GSC1314-0530: An ultra-short period eclipsing low mass binary system
Published: 2014-08-31T00:00:00Z

Proposal ID	072018
Title	GSC1314-0530: An ultra-short period eclipsing low mass binary system
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720180101
DOI	https://doi.org/10.5270/esa-55q5x24
Principal Investigator, PI	Prof Jurgen Schmitt
Abstract	We propose the first detailed X-ray study of the eclipsing M-dwarf binaryGSC1314-0530, consisting of two M dwarfs with masses 0.51 and 0.26 solar masses;its period of 0.192636 days makes GSC1314-0530 the M-dwarf system with theshortest known period, with the larger of the components almost filling itsRoche lobe. We propose a 35 ksec observation with XMM-Newton to carry out thefirst in-depth X-ray study of this system with the aim to characterize theactivity properties of this remarkable system and to study the rotationalmodulation of its X-ray flux.
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 X-ray and UV emission of the ultrashort-period low-mass eclipsing binary system BX Trianguli \|Perdelwitz V. Czesla S. et al. \| A&A \| 619-138 \| 2018 \| 2018A&A...619A.138P \| http://ui.adsabs.harvard.edu/#abs/2018A&A...619A.138P 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 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 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	2013-07-19T00:15:05Z/2013-07-19T13:48:25Z
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	2014-08-31T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "XMM-Newton", "gsc1314 0530", "rotational modulation", "roche lobe", "depth xray", "solar masses", "activity properties", "xray flux", "xmm newton", "dwarf system", "makes gsc1314 0530"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Jurgen Schmitt, 2014, 'GSC1314-0530: An ultra-short period eclipsing low mass binary system', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-55q5x24