A dataset provided by the European Space Agency

Name 065338
Title Mapping the Timing - Spectral Correlations in NGC 5408 X-1
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380701

DOI 10.5270/esa-4c2qkow
Author Dr Tod Strohmayer
Description We propose new, deep EPIC observations of the ULX NGC 5408 X-1. Our previous observations reveal a pattern of timing and spectral behavior very analogous to that seen in Galactic black holes, but with longer timescale and higher luminosity, strongly indicative of a ~1000 solar mass black hole in X-1. With new exposures we will 1) map out the timing - spectral correlations to enable more rigorous comparison with Galactic systems. 2) Search for analogs of the high frequency QPOs in Galactic black holes in the Steep Power-law State. 3) Search for relativistically broadened Fe lines.
Publication A Multi-epoch Timing and Spectral Study of the Ultraluminous X-Ray NGC 5408 X-1 with XMM-Newton . Dheeraj, Pasham R., Strohmayer, Tod E., . ApJ . 753-139 . 2012 . 2012ApJ...753..139D ,
The ultraluminous state revisited: fractional variability and spectral shape as diagnostics of super-Eddington accretion . Sutton, Andrew D., Roberts, Timothy P., . MNRAS . 435-1758 . 2013 . 2013MNRAS.435.1758S ,
The Local Environment of Ultraluminous X-Ray Sources Viewed by XMM-Newton.s Optical Monitor . Berghea, C. T., Dudik, R. P., et all. . ApJ . 776-100 . 2013 . 2013ApJ...776..100B ,
X-ray variability and energy spectra from NGC 5408 X-1 with XMM-Newton . Caballero-Garcia, M. D., Belloni, T. M., . MNRAS . 435-2665 . 2013 . 2013MNRAS.435.2665C ,
Time lags in the ultraluminous X-ray source NGC 5408 X-1: implications for the black hole mass . De Marco, B., Ponti, G., et all. . MNRAS . 436-3782 . 2013 . 2013MNRAS.436.3782D ,
Revisiting Putative Cool Accretion Disks in Ultraluminous X-Ray Sources . Miller, J. M., Walton, D. J., et all. . ApJ . 776-36 . 2013 . 2013ApJ...776L..36M ,
Broad absorption features in wind-dominated ultraluminous X-ray sources? . Middleton, Matthew J., Walton, Dominic J., et all. . MNRAS . 438-51 . 2014 . 2014MNRAS.438L..51M ,
Ultraluminous X-ray sources: a deeper insight into their spectral evolution . Pintore, Fabio, Zampieri, Luca, et all. . MNRAS . ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2010-07-17T03:12:59Z/2011-01-30T02:55:08Z
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 2012-02-18T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-02-18T00:00:00Z, 065338, 17.56_20190403_1200. https://doi.org/10.5270/esa-4c2qkow