A dataset provided by the European Space Agency

Name 065505
Title Discovery of a QPO in the NGC55 ULX?


DOI 10.5270/esa-czkxp53
Description We request a long (125ks) XMM-Newton observation of the ULX in the nearby galaxy NGC55. Previous short observations have revealed several unique aspects of this ULX. The temporal behavior of the ULX suggests a QPO at 1.5mHz and a power spectrum break. Such temporal features have been observed only for three other ULXs. Moreover, the source undergoes frequent spectral transitions making it a unique ULX where characteristic temporal behavior can be studied in conjunction with spectral transitions. Such studies are crucial to understanding the differences-similarities between ULX and Galactic X-ray binaries. Furthermore, the ULX exhibits a series of strange and unexplained X-ray dips of duration ~200s, whose nature can be revealed in spectral analysis of co-added dip data.
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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 ,
X-ray outbursts from a new transient in NGC 55 . Jithesh, V., Wang, Zhongxiang, . MNRAS . 448-1973 . 2015 . 2015MNRAS.448.1973J ,
A spectral-timing model for ULXs in the supercritical regime . Middleton, Matthew J., Heil, Lucy, et all. . MNRAS . 447-3243 . 2015 . 2015MNRAS.447.3243M ,
Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra . Anderson, Michael E., Churazov, Eugene, . MNRAS . 452-3905 . 2015 . 2015MNRAS.452.3905A ,
Diagnosing the accretion flow in ultraluminous X-ray sources using soft X-ray atomic features . Middleton, Matthew J., Walton, Dominic J., et all. . MNRAS . 454-3134 . 2015 . 2015MNRAS.454.3134M ,
Transient X-Ray Source Population in the Magellanic-type Galaxy NGC 55 . Jithesh, V., Wang, Zhongxiang, . ApJ . 821-24 . 2016 . 2016ApJ...821...24J ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Pulsator-like Spectr...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-05-24T07:25:00Z/2010-05-25T18:48:57Z
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 2011-06-16T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-06-16T00:00:00Z, 065505, 17.56_20190403_1200. https://doi.org/10.5270/esa-czkxp53