A dataset provided by the European Space Agency

Name 069390
Title Searching for pulsations in the SFXTs IGR J17354-3255 and SAX J1818.6-1703
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693900101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693900201

DOI https://doi.org/10.5270/esa-to2jfhr
Author Mr Sebastian Drave
Description The Supergiant Fast X-ray Transients (SFXTs) IGR J17354-3255 and SAX
J1818.6-1703 are in the central region of the SFXT orbital period range and both
show a high .recurrence. of periastron emission. Here we propose to perform
sensitive, soft X-ray observations during the system periastron passages for the
first time. These precisely targeted observations will maximise the probability
of detecting pulsations in these systems and also allow us to place firm
constraints on the stellar wind geometry within them. These measurements are
essential to advance our current understanding of SFXTs, having the potential to
alter the way in which we view the class as a whole and whether they can indeed
be considered a single class of systems at all.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-03-15T13:04:56Z/2013-03-21T21:24:54Z
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 2014-04-12T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Mr Sebastian Drave, 2014, 069390, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-to2jfhr