A dataset provided by the European Space Agency

Name: Mapping the Timing - Spectral Correlations in NGC 5408 X-1
Published: 2012-02-18T00:00:00Z

Proposal ID	065338
Title	Mapping the Timing - Spectral Correlations in NGC 5408 X-1
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653380701
DOI	https://doi.org/10.5270/esa-4c2qkow
Principal Investigator, PI	Dr Tod Strohmayer
Abstract	We propose new, deep EPIC observations of the ULX NGC 5408 X-1. Our previousobservations reveal a pattern of timing and spectral behavior very analogous tothat seen in Galactic black holes, but with longer timescale and higherluminosity, strongly indicative of a virgul1000 solar mass black hole in X-1. Withnew exposures we will 1) map out the timing - spectral correlations to enablemore rigorous comparison with Galactic systems. 2) Search for analogs of thehigh frequency QPOs in Galactic black holes in the Steep Power-law State. 3)Search for relativistically broadened Fe lines.
Publications	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 \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/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 al. \| ApJ \| 776-100 \| 2013 \| 2013ApJ...776..100B \| http://ui.adsabs.harvard.edu/#abs/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 \| http://ui.adsabs.harvard.edu/#abs/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 al. \| MNRAS \| 436-3782 \| 2013 \| 2013MNRAS.436.3782D \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.436.3782D Revisiting Putative Cool Accretion Disks in Ultraluminous X-Ray Sources \|Miller, J. M., Walton, D. J., et al. \| ApJ \| 776-36 \| 2013 \| 2013ApJ...776L..36M \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...776L..36M Broad absorption features in wind-dominated ultraluminous X-ray sources? \|Middleton, Matthew J., Walton, Dominic J., et al. \| MNRAS \| 438-51 \| 2014 \| 2014MNRAS.438L..51M \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438L..51M Ultraluminous X-ray sources: a deeper insight into their spectral evolution \|Pintore, Fabio, Zampieri, Luca, et al. \| MNRAS \| 439-3461 \| 2014 \| 2014MNRAS.439.3461P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.439.3461P 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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y A spectral-timing model for ULXs in the supercritical regime \|Middleton, Matthew J., Heil, Lucy, et al. \| MNRAS \| 447-3243 \| 2015 \| 2015MNRAS.447.3243M \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.447.3243M X-ray time lags and non-linear variability in the ultraluminous X-ray sources NGC 5408 X-1 and NGC 6946 X-1 \|Hernandez-Garcia, L., Vaughan, S., et al. \| MNRAS \| 453-2877 \| 2015 \| 2015MNRAS.453.2877H \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.453.2877H Optically thick outflows in ultraluminous supersoft sources \|Urquhart, R., Soria, R., \| MNRAS \| 456-1859 \| 2016 \| 2016MNRAS.456.1859U \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.456.1859U Resolved atomic lines reveal outflows in two ultraluminous X-ray sources \|Pinto, Ciro, Middleton, Matthew J., \| Natur \| 533-64 \| 2016 \| 2016Natur.533...64P \| http://ui.adsabs.harvard.edu/#abs/2016Natur.533...64P The Rotation of the Hot Gas around the Milky Way \|Hodges-Kluck, Edmund J., Miller, Matthew J., \| ApJ \| 822-21 \| 2016 \| 2016ApJ...822...21H \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...822...21H The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F The thin and medium filters of the EPIC camera on-board XMM-Newton: measured performance after more than 15 years of operation \|Barbera, Marco, Gastaldello, Fabio, et al. \| ExA \| 42-179 \| 2016 \| 2016ExA....42..179B \| http://ui.adsabs.harvard.edu/#abs/2016ExA....42..179B Pulsator-like Spectra from Ultraluminous X-Ray Sources and the Search for More Ultraluminous Pulsars \|Pintore, F., Zampieri, L., et al. \| ApJ \| 836-113 \| 2017 \| 2017ApJ...836..113P \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...836..113P Analysis of Quasi-periodic Oscillations and Time Lag in Ultraluminous X-Ray Sources with XMM-Newton \|Li, Zi-Jian, Xiao, Guang-Cheng, et al. \| ApJ \| 839-19 \| 2017 \| 2017ApJ...839...19L \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...839...19L From ultraluminous X-ray sources to ultraluminous supersoft sources: NGC 55 ULX, the missing link \|Pinto, C., Alston, W., et al. \| MNRAS \| 468-2865 \| 2017 \| 2017MNRAS.468.2865P \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468.2865P Ultrafast outflows in ultraluminous X-ray sources \|Pinto, C., Fabian, A., et al. \| AN \| 338-234 \| 2017 \| 2017AN....338..234P \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..234P First results from the use of the relativistic and slim disc model SLIMULX in XSPEC \|Caballero-Garcia, M. D., Bursa, M., et al. \| CoSka \| 47-84 \| 2017 \| 2017CoSka..47...84C \| http://ui.adsabs.harvard.edu/#abs/2017CoSka..47...84C A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw, H. P., Roberts, T. P., et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E Ultraluminous X-ray sources with flat-topped noise and QPO \|Atapin, Kirill, Fabrika, Sergei, \| MNRAS \| 486-2766 \| 2019 \| 2019MNRAS.486.2766A \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.486.2766A A Multi-epoch Timing and Spectral Study of the Ultraluminous X-Ray NGC 5408 X-1 with XMM-Newton \|Pasham, Dheeraj R., Strohmayer, Tod E., \| ApJ \| 753-139 \| 2012 \| 2012ApJ...753..139P \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...753..139P Thermal stability of winds driven by radiation pressure in super-Eddington accretion discs \|Pinto, C., Mehdipour, M., et al. \| MNRAS \| 491-5702 \| 2020 \| 2020MNRAS.491.5702P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491.5702P Linking Soft Excess in Ultraluminous X-Ray Sources with Optically Thick Wind Driven by Supercritical Accretion \|Qiu, Yanli, Feng, Hua, \| ApJ \| 906-36 \| 2021 \| 2021ApJ...906...36Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...906...36Q Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z X-ray reverberation models of the disc wind in ultraluminous X-ray source NGC 5408 X-1 \|Luangtip, W., Chainakun, P., et al. \| MNRAS \| 507-6094 \| 2021 \| 2021MNRAS.507.6094L \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.6094L Ionized emission and absorption in a large sample of ultraluminous X-ray sources \|Kosec, P., Pinto, C., et al. \| MNRAS \| 508-3569 \| 2021 \| 2021MNRAS.508.3569K \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.508.3569K The impact of precession on the observed population of ULXs \|Khan, Norman, Middleton, Matthew J., et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows, R., Comerford, Julia M., et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S Winds in ultraluminous X\\u2011ray sources: New challenges \|Pinto, C., Kosec, P., \| AN \| 344-20220134 \| 2023 \| 2023AN....34420134P \| http://ui.adsabs.harvard.edu/#abs/2023AN....34420134P Ultraluminous X-ray sources \|King, Andrew, Lasota, Jean-Pierre, \| NewAR \| 96-101672 \| 2023 \| 2023NewAR..9601672K \| http://ui.adsabs.harvard.edu/#abs/2023NewAR..9601672K Unveiling the accretion scenario of BH-ULXs using XMM-Newton observations \|Majumder, Seshadri, Das, Santabrata, et al. \| MNRAS \| 526-2086 \| 2023 \| 2023MNRAS.526.2086M \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.2086M The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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 Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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
Keywords	"NGC 5408", "frequency qpos", "solar mass blackhole", "galactic blackhole", "galactic systems", "power law", "deep epic", "galactic black holes", "EPIC", "spectral correlations", "ngc 5408 x"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Tod Strohmayer, 2012, 'Mapping the Timing - Spectral Correlations in NGC 5408 X-1', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-4c2qkow