A dataset provided by the European Space Agency

Name: Observation of the black hole candidate X-ray binary Swift J1357.2 0933 in quies
Published: 2014-09-01T00:00:00Z

Proposal ID	072432
Title	Observation of the black hole candidate X-ray binary Swift J1357.2 0933 in quies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724320101
DOI	https://doi.org/10.5270/esa-sgsr6cu
Principal Investigator, PI	Ms Montserrat Armas Padilla
Abstract	We propose a 40 ksec XMM Newton observation of the low mass X-ray binary blackhole system Swift J1357.2 0933 in the quiescent state. The low column densitytowards the source makes it possible to obtain its quiescent lumi- nosity downto LX virgul1E30 ergs s-1. This limit, together with its short orbital period of 2.8hours makes it possible to test the ADAF interpretation for emission inquiescent black holes systems by testing the quiescent luminosity-orbital periodcorrelation in the unexplored regime of very short orbital periods.
Publications	Swift J1357.2-0933: the faintest black hole? \|Armas Padilla, M., Wijnands, R., et al. \| MNRAS \| 444-902 \| 2014 \| 2014MNRAS.444..902A \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444..902A 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 Modelling the effect of absorption from the interstellar medium on transient black hole X-ray binaries \|Eckersall, A. J., Vaughan, S., \| MNRAS \| 471-1468 \| 2017 \| 2017MNRAS.471.1468E \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1468E 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 omnipresent flux-dependent optical dips of the black hole transient Swift J1357.2\\u22120933 \|Panizo-Espinar, G., Mu\\u00f1oz-Darias, T., et al. \| A&A \| 682-A19 \| 2024 \| 2024A&A...682A..19P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...682A..19P 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2013-07-10T11:41:21Z/2013-07-11T02:16:21Z
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	2014-09-01T00:00:00Z
Keywords	"short orbital periods", "short orbital period", "XMM", "unexplored regime", "J1357.2", "1e30 ergs", "source makes", "quiescent blackhole systems", "xmm newton", "quiescent lumi nosity"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Ms Montserrat Armas Padilla, 2014, 'Observation of the black hole candidate X-ray binary Swift J1357.2 0933 in quies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-sgsr6cu