A dataset provided by the European Space Agency

Name 000862
Title The Bursting, Dipping, Eclipsing, X-ray Transient MXB 1659-298
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0008620601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0008620701

DOI 10.5270/esa-8bc6pgg
Author Dr Arvind Parmar
Description The eclipsing, dipping, bursting X-ray transient MXB1659-298 is currently undergoing an outburst, the first detected in 21 years. If this outburst continues into AO1, or if the source undergoes another outburst during AO1 then we propose a single 'TOO-like. observation of this object. This would be the first X-ray observation with instruments other than proportional counters and will yield a wealth of information about the eclipses, the accretion disk corona and the dipping activity. An unconstrained observation, slightly longer than two 7.1 hr orbital periods is requested to ensure that two complete eclipses are observed.
Publication An XMM-Newton study of the X-ray binary MXB 1659-298 and the discovery of narrow X-ray absorption lines . Sidoli, L., Oosterbroek, T., et all. . A&A . 379-540 . 2001 . 2001A&A...379..540S ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
Spectral changes during dipping in low-mass X-ray binaries due to highly-ionized absorbers . Diaz Trigo, M., Parmar, A. N., et all. . A&A . 445-179 . 2006 . 2006A&A...445..179D ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog . Lin, Dacheng, Webb, Natalie A., . ApJ . 756-27 . 2012 . 2012ApJ...756...27L , ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-03-22T00:04:27Z/2001-02-20T16:52:39Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2004-06-05T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2004-06-05T00:00:00Z, 000862, 17.56_20190403_1200. https://doi.org/10.5270/esa-8bc6pgg