A dataset provided by the European Space Agency

Name 076169
Title Unveiling the nature of newly discovered X-ray pulsators
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761690301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761690401

DOI 10.5270/esa-029zn1z
Author Prof GianLuca Israel
Description In the largest ever systematic search in soft X-rays for coherent periodicities [about 440,000 light curves of sources serendipitously detected by the Swift X-Ray Telescope (XRT) and the Chandra Advanced CCD Imaging Spectrometer (ACIS)] we have discovered so far (the project is still on-going) almost 40 new X-ray pulsators. In this proposal we ask for XMM-Newton follow-up observations for four of them, which either show unusual characteristics or their properties are suggesting the presence of an accreting neutron star. The requested observations will allow us to unveil their nature and test magnetic gating accretion scenarios, a regime which has remained unexplored so far.
Publication XMM-Newton discovery of mHz quasi-periodic oscillations in the high-mass X-ray binary IGR J19140+0951 . Sidoli, L., Esposito, P., et all. . MNRAS . 460-3637 . 2016 . 2016MNRAS.460.3637S ,
The Chandra ACIS Timing Survey Project: glimpsing a sample of faint X-ray pulsators . Israel, G. L., Esposito, P., et all. . MNRAS . 462-4371 . 2016 . 2016MNRAS.462.4371I ,
Supergiant fast X-ray transients versus classical supergiant high mass X-ray binaries: Does the difference lie in the companion wind? . Pradhan, P., Bozzo, E., . A&A . 610-50 . 2018 . 2018A&A...610A..50P ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2015-10-26T17:04:35Z/2016-02-06T18:09:35Z
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 2017-02-26T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2017-02-26T23:00:00Z, 076169, 17.56_20190403_1200. https://doi.org/10.5270/esa-029zn1z