A dataset provided by the European Space Agency

Name 074405
Title Extreme ULXs: super-Eddington accretors, or intermediate-mass black holes
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744050101

DOI 10.5270/esa-9no2cm6
Author Dr Fabio Pintore
Description Ultraluminous X-ray sources with luminosities up to 2e40 erg-s are now regarded as likely super-Eddington accretors powered by stellar mass black holes, and those above 1e41 erg-s may be good intermediate-mass black hole (IMBH) candidates. However, the few objects lying between these ranges have an uncertain nature, and remain poorly studied. Here, we propose a new deep observation of one such object located within 20 Mpc. We will use the high quality EPIC data to determine whether its spectrum shows the characteristic signatures of the ultraluminous state, indicative of super-Eddington accretion onto large stellar black holes, or whether it appears consistent with the hard power-law spectra and >10% fractional variability of an IMBH in the hard state.
Publication The ultraluminous X-ray source NGC 5643 ULX1: a large stellar mass black hole accreting at super-Eddington rates? . Pintore, Fabio, Zampieri, Luca, et all. . MNRAS . 459-455 . 2016 . 2016MNRAS.459..455P ,
NuSTAR and XMM-Newton observations of the ultraluminous X-ray source NGC 5643 X-1 . Krivonos, Roman, Sazonov, Sergey, . MNRAS . 463-756 . 2016 . 2016MNRAS.463..756K ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Pulsator-like Spectra from Ultraluminous X-Ray Sources and the Search for More Ultraluminous Pulsars . Pintore, F., Zampieri, L., et all. . ApJ . 836-113 . 2017 . 2017ApJ...836..113P ,
Searching for outflows in ultraluminous X-ray sources through high-resolution X-ray spectroscopy . Kosec, P., Pinto, C., et all. . MNRAS . 473-5680 . 2018 . 2018MNRAS.473.5680K ,
Spectral Properties of Heavily Obscured Seyfert Galaxies from the INTEGRAL All-Sky Survey . Semena, A. N., Sazonov, S. Yu., . AstL . 45-490 . 2019 . 2019AstL...45..490S ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-08-27T01:48:16Z/2014-08-28T10:16:36Z
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 2015-09-19T22:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-09-19T22:00:00Z, 074405, 17.56_20190403_1200. https://doi.org/10.5270/esa-9no2cm6