A dataset provided by the European Space Agency

Name 060561
Title Disentangling the disks in hard state black hole X-ray binaries


DOI 10.5270/esa-9yodhoq
Author Dr Phil Uttley
Description We propose up to 3 TOO EPIC-pn observations of the hard states of the BHXRBs Cyg X-1, GX 339-4 and SWIFT J1753.5-0127, to be triggered by a significant change in their timing signatures with respect to those seen in earlier hard state observations. In this way, we will confirm or disprove the standard picture of the hard state where correlated timing and spectral properties are caused by truncation of the accretion disk. We will use rms-spectra to disentangle the intrinsic and reprocessed contributions to disk thermal emission, and determine whether the enhanced disk variability seen on longer time-scales is associated with the low-frequency Lorentzian in the PSD, which would for the first time identify this key timing signature with the disk.
Publication Joint spectral-timing modelling of the hard lags in GX 339-4: constraints on reflection models . Cassatella, P., Uttley, P., et all. . MNRAS . 422-2407 . 2012 . 2012MNRAS.422.2407C ,
Probing the Environment of Accreting Compact Objects . Hanke, Manfred, . PhDT . 0-9 . 2011 . 2011PhDT.........9H ,
Accretion flow diagnostics with X-ray spectral timing: the hard state of SWIFT J1753.5-0127 . Cassatella, P., Uttley, P., . MNRAS . 427-2985 . 2012 . 2012MNRAS.427.2985C ,
Interstellar medium composition through X-ray spectroscopy of low-mass X-ray binaries . Pinto, C., Kaastra, J. S., et all. . A&A . 551-25 . 2013 . 2013A&A...551A..25P ,
Ubiquitous equatorial accretion disc winds in black hole soft states . Ponti, G., Fender, R. P., et all. . MNRAS . 422-11 . 2012 . 2012MNRAS.422L..11P ,
The soft component and the iron line as signatures of the disc inner radius in Galactic black hole binaries . Kolehmainen, Mari, Done, Chris, . MNRAS . 437-316 . 2014 . 2014MNRAS.437..316K ,
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 ,
The truncated and evolving inner accretion disc of the black hole GX 339-4 . Plant, D. S., Fender, R. P., et all. . A&A . 573-120 . 2015 . 2015A&A...573A.120P ,
Tracing the Reverberat...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-03-26T07:31:44Z/2009-12-02T12:53:18Z
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 2010-12-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2010-12-17T00:00:00Z, 060561, 17.56_20190403_1200. https://doi.org/10.5270/esa-9yodhoq