A dataset provided by the European Space Agency

Name 040292
Title A Search for Pulsations from INTEGRAL Sources in the Norma Region
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402920101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0402920201

DOI 10.5270/esa-ja6rkkd
Author Dr John Tomsick
Description We propose to search for X-ray pulsations from four of the hard X-ray IGR sources that have been discovered by the INTEGRAL satellite. Our targets are in the Norma region of the Galaxy and are candidate neutron star High-Mass X-Ray Binaries. The sources are persistent in X-rays as evidenced by strong detections of all four during brief (~5 ks) Chandra observations that occurred during 2005 April-July. The proposed observations are critical to definitively identify these sources as neutron star X-ray binaries. These studies are important for characterizing the population of IGR sources, leading to a better understanding of binary evolution and compact object formation.
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Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
An XMM-Newton view of FeKalpha in high-mass X-ray binaries . Gimenez-Garcia, A., Torrejon, J. M., et all. . A&A . 576-108 . 2015 . 2015A&A...576A.108G ,
Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters . Xiao, Weike, Chen, Chen, et all. . MNRAS . 432-41 . 2013 . 2013MNRAS.432L..41X ,
The Million Optical - Radio-X-ray ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2006-08-17T16:11:15Z/2007-03-13T20:25:36Z
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 2008-03-30T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-03-30T00:00:00Z, 040292, 17.56_20190403_1200. https://doi.org/10.5270/esa-ja6rkkd