A dataset provided by the European Space Agency

Name 072481
Title X-ray Study of Ultraluminous X-ray Sources with XMM-Newton and NuSTAR
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724810101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724810201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724810301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0724810401

DOI 10.5270/esa-8k4ssoz
Author Prof Fiona Harrison
Description We propose to continue the simultaneous XMM+NuSTAR observing program for ultraluminous X-ray sources (ULXs) initiated in the previous observing cycle, with observations of two further sources of interest, Holmberg II X-1 and NGC5907 ULX. The bright X-ray emission from ULX binaries greatly exceeds the Eddington luminosity for a spherically accreting stellar-mass compact object, and understanding why this is so is one of the biggest mysteries in high energy astrophysics. Combined, XMM-Newton and NuSTAR will obtain high-quality spectra and timing measurements from 0.3 30 keV, providing powerful probes for understanding the accretion modes and nature of the central BHs.
Publication NuSTAR and XMM-Newton Observations of the Extreme Ultraluminous X-Ray Source NGC 5907 ULX1: A Vanishing Act . Walton, D. J., Harrison, F. A., et all. . ApJ . 799-122 . 2015 . 2015ApJ...799..122W ,
Constraining the Milky Way.s Hot Gas Halo with O VII and O VIII Emission Lines . Miller, Matthew J., Bregman, Joel N., . ApJ . 800-14 . 2015 . 2015ApJ...800...14M ,
NuSTAR, XMM-Newton, and Suzaku Observations of the Ultraluminous X-Ray Source Holmberg II X-1 . Walton, D. J., Middleton, M. J., et all. . ApJ . 806-65 . 2015 . 2015ApJ...806...65W ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
A new characterization of the Compton process in the ULX spectra . Kobayashi, S., Nakazawa, K., . AN . 337-479 . 2016 . 2016AN....337..479K ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Spectral Changes in the Hyperluminous Pulsar in NGC 5907 as a Function of Super-orbital Phase . Furst, F., Walton, D. J., et all. . ApJ . 834-77 . 2017 . 2017ApJ...834...77F ,
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 ,
AGN spectra...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-09-09T06:16:17Z/2013-11-13T01:42:52Z
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 2014-11-26T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-11-26T00:00:00Z, 072481, 17.56_20190403_1200. https://doi.org/10.5270/esa-8k4ssoz