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
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	2025-01-27
Keywords	"roche lobe", "depth xray", "solar masses", "activity properties", "makes gsc1314 0530", "xmm newton", "XMM-Newton", "xray flux", "XMM", "gsc1314 0530", "dwarf system", "rotational modulation"
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